[1]:
import matplotlib.pyplot as plt
import numpy as np
import scipy as sp
np.seterr(all="ignore")
from threeML import *
from threeML.io.package_data import get_path_of_data_file
from threeML.io import update_logging_level
from threeML.utils.data_download.Fermi_LAT.download_LAT_data import LAT_dataset
from astropy.io import fits as pyfits
SMALL_SIZE = 15
MEDIUM_SIZE = 15
BIGGER_SIZE = 20
plt.rc("font", size=SMALL_SIZE) # controls default text sizes
plt.rc("axes", titlesize=SMALL_SIZE) # fontsize of the axes title
plt.rc("axes", labelsize=MEDIUM_SIZE) # fontsize of the x and y labels
plt.rc("xtick", labelsize=SMALL_SIZE) # fontsize of the tick labels
plt.rc("ytick", labelsize=SMALL_SIZE) # fontsize of the tick labels
plt.rc("legend", fontsize=SMALL_SIZE) # legend fontsize
plt.rc("figure", titlesize=BIGGER_SIZE) # fontsize of the figure title
# This if you want to toggle different type of logging level.
update_logging_level("INFO")
log.error("error")
log.info("info")
log.debug("debug")
00:20:17 WARNING The naima package is not available. Models that depend on it will not be functions.py:50 available
WARNING The GSL library or the pygsl wrapper cannot be loaded. Models that depend on it functions.py:71 will not be available.
00:20:18 WARNING The ebltable package is not available. Models that depend on it will not be absorption.py:36 available
00:20:20 ERROR error 3699701126.py:29
INFO info 3699701126.py:30
GtBurst
Gtburst contains all the classes and methods to perform Fermi LAT data. It internally uses the official fermitools software. Here an example to list the IRFS available:
[2]:
from GtBurst import IRFS
irfs = IRFS.IRFS.keys()
print(irfs)
odict_keys(['p7rep_transient', 'p7rep_source', 'p7rep_clean', 'p7rep_ultraclean', 'p8r2_transient100e', 'p8r2_transient100', 'p8r2_transient020e', 'p8r2_transient020', 'p8r2_transient010e', 'p8r2_transient010', 'p8r2_source', 'p8r2_clean', 'p8r2_ultraclean', 'p8r2_ultracleanveto', 'p8r2_transient100s', 'p8r2_transient015s', 'p8_transient100e', 'p8_transient100', 'p8_transient020e', 'p8_transient020', 'p8_transient010e', 'p8_transient010', 'p8_source', 'p8_clean', 'p8_ultraclean', 'p8_ultracleanveto', 'p8_sourceveto', 'p8_transient100s', 'p8_transient015s'])
The LAT Transient Builder
Let’s see how to make a plug in for the unbinned analysis of Fermi LAT data. First we use the information form a triggered GRB to obtain MET, RA and DEC, that are needed for the analysis.
[3]:
from GtBurst.TriggerSelector import TriggerSelector
myFavoriteGRB = "bn190114873"
def findGRB(grb_name):
a = TriggerSelector()
a.downloadList()
myGRB = {}
for x in a.data:
if x[0] == myFavoriteGRB:
myGRB["MET"] = float(x[1])
myGRB["RA"] = float(x[3])
myGRB["DEC"] = float(x[4])
myGRB["ERR"] = float(x[5])
return myGRB
pass
return None
[4]:
myGRB = findGRB(myFavoriteGRB)
print(myGRB)
{'MET': 569192227.626, 'RA': 54.51, 'DEC': -26.939, 'ERR': 0.05}
Then, we download LAT data and we build the transient builder, we want to analyze 1000 seconds since the trigger. Let’s start download the data:
[5]:
tstart = 0
tstop = 1000
[6]:
myLATdataset = LAT_dataset()
myLATdataset.make_LAT_dataset(
ra=myGRB["RA"],
dec=myGRB["DEC"],
radius=12,
trigger_time=myGRB["MET"],
tstart=tstart,
tstop=tstop,
data_type="Extended",
destination_directory=".",
Emin=100.0,
Emax=10000.0,
) # Energies are MeV (this is from 100 MeV to 10 GeV)
00:20:38 INFO Query parameters: download_LAT_data.py:262
INFO coordfield = 54.5100,-26.9390 download_LAT_data.py:266
INFO coordsystem = J2000 download_LAT_data.py:266
INFO shapefield = 12 download_LAT_data.py:266
INFO timefield = 569192227.626,569193227.626 download_LAT_data.py:266
INFO timetype = MET download_LAT_data.py:266
INFO energyfield = 100.000,10000.000 download_LAT_data.py:266
INFO photonOrExtendedOrNone = Extended download_LAT_data.py:266
INFO destination = query download_LAT_data.py:266
INFO spacecraft = checked download_LAT_data.py:266
INFO Query ID: 86ad4d2b3b3e5065f0f0a976e6fc8315 download_LAT_data.py:271
INFO Estimated complete time for your query: 15 seconds download_LAT_data.py:427
INFO If this download fails, you can find your data at download_LAT_data.py:436 https://fermi.gsfc.nasa.gov/cgi-bin/ssc/LAT/QueryResults.cgi?id=L2210042 020398D96CEF299 (when ready)
00:20:50 INFO Downloading FT1 and FT2 files... download_LAT_data.py:526
00:20:54 WARNING Only one FT1 file provided. Skipping the merge... download_LAT_data.py:98
Writing ./bn190114873/gll_cspec_tr_bn190114873_v00.rsp...
time -p gtselect infile=./bn190114873/gll_ft1_tr_bn190114873_v00.fit outfile=__temp_ft1.fits ra=54.51 dec=-26.939 rad=15.0 tmin=569192226.626 tmax=569193228.626 emin=10.0 emax=300000.0 zmin=0.0 zmax=110.0 evclass="INDEF" evtype="INDEF" convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Writing ./bn190114873/gll_cspec_tr_bn190114873_v00.pha...
* Get energy binning from the response matrix...
done.
* Run gtbindef and gtbin and bin in energy and time...
time -p gtbindef bintype="E" binfile=__ebins.txt outfile=__energyBins.fits energyunits="keV" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbindef version HEAD
real 0.20
user 0.01
sys 0.01
time -p gtbin evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/__temp_ft1.fits scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=__gtllebin__pha2.pha algorithm="PHA2" ebinalg="FILE" emin=30.0 emax=200000.0 ebinfile=__energyBins.fits tbinalg="LIN" tstart=569192227.626 tstop=569193227.626 dtime=4.096 tbinfile=NONE coordsys="CEL" axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=1 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 2.71
user 2.31
sys 0.38
done.
* Transform gtbin output in CSPEC format...
done.
* Updating keywords in the headers of the CSPEC file...
done.
gtllebin done!
WARNING: VerifyWarning: Card is too long, comment will be truncated. [astropy.io.fits.card]
We want perform a time resolved analysis. So, first we look at the data. We can play with the ROI selection and the cut.
[7]:
roi = 10
zmax = 110.0
thetamax = 180.0
irfs = "p8_transient020e"
strategy = "time"
myLATdataset.extract_events(roi, zmax, irfs, thetamax, strategy="time")
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192227.626 tstop=569193227.626 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192227.626 tmax=569193227.626 emin=100.0 emax=10000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 251 events.
00:20:57 INFO Extracted 251 events download_LAT_data.py:669
[8]:
%matplotlib inline
event_file = pyfits.open(myLATdataset.filt_file)
event_times = sorted(event_file["EVENTS"].data["TIME"] - myGRB["MET"])
intervals = event_times[0::10]
_ = plt.hist(event_times)
_ = plt.hist(event_times, intervals, histtype="step")
# plt.show()
tstarts and tstops are defined as strings, with somma separated values for the starts and the ends of the time bins: For example tsrats=“0,1,10” and tstops=“1,10,20”. To convert arrays in string we use these few lines of code:
[9]:
tstarts = tstops = ""
for t0, t1 in zip(intervals[:-1], intervals[1:]):
tstarts += "%.4f," % t0
tstops += "%.4f," % t1
pass
tstarts = tstarts[:-1].replace("-", "\\-")
tstops = tstops[:-1].replace("-", "\\-")
We can now make an instance the LAT transient builder
[10]:
analysis_builder = TransientLATDataBuilder(
myLATdataset.grb_name,
outfile=myLATdataset.grb_name,
roi=roi,
tstarts=tstarts,
tstops=tstops,
irf=irfs,
zmax=zmax,
galactic_model="template",
particle_model="isotr template",
datarepository=".",
)
df = analysis_builder.display(get=True)
outfile 190114873
roi 10
tstarts 2.6996,3.6358,3.9968,4.4024,4.7375,5.0909,5.54...
tstops 3.6358,3.9968,4.4024,4.7375,5.0909,5.5471,5.98...
zmax 110.0
emin 100.0
emax 100000.0
irf p8_transient020e
galactic_model template
particle_model isotr template
source_model PowerLaw2
tsmin 20.0
strategy time
thetamax 180.0
spectralfiles no
liketype unbinned
optimizeposition no
datarepository .
ltcube
expomap
ulphindex -2
flemin 100
flemax 10000
fgl_mode fast
filter_GTI False
likelihood_profile False
remove_fits_files False
dtype: object
[11]:
tstops
[11]:
'3.6358,3.9968,4.4024,4.7375,5.0909,5.5471,5.9896,6.3998,6.6889,7.0117,7.2936,7.7731,8.2167,8.8763,9.6573,10.5680,12.0568,14.6165,17.7834,21.4962,30.0798,40.8747,48.7118,73.7262,172.5754'
The run method will run (using gtburst) all the fermitools needed to obtain the needed file for the likelihood analysis (livetimecubes, exposure maps. It will also perfom a simple likelihood analysis with the standard likelihood of the fermitools (pylikelihood). The dataproducts created here will be used by threeML to make the fit.
[12]:
LAT_observations = analysis_builder.run(include_previous_intervals=True)
Changing permission to /usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/scripts/doTimeResolvedLike.py
Changing permission to /usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtdiffrsp_mp.py
Changing permission to /usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py
Changing permission to /usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtltcube_mp.py
Changing permission to /usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gttsmap_mp.py
00:20:58 INFO About to run the following command: lat_transient_builder.py:636 /usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermi tools/GtBurst/scripts/doTimeResolvedLike.py 190114873 --outfile '190114873' --roi 10.000000 --tstarts '2.6996,3.6358,3.9968,4.4024,4.7375,5.0909,5.5471,5.9896,6.3998,6.68 89,7.0117,7.2936,7.7731,8.2167,8.8763,9.6573,10.5680,12.0568,14.6165 ,17.7834,21.4962,30.0798,40.8747,48.7118,73.7262' --tstops '3.6358,3.9968,4.4024,4.7375,5.0909,5.5471,5.9896,6.3998,6.6889,7.01 17,7.2936,7.7731,8.2167,8.8763,9.6573,10.5680,12.0568,14.6165,17.783 4,21.4962,30.0798,40.8747,48.7118,73.7262,172.5754' --zmax 110.000000 --emin 100.000000 --emax 100000.000000 --irf 'p8_transient020e' --galactic_model 'template' --particle_model 'isotr template' --source_model 'PowerLaw2' --tsmin 20.000000 --strategy 'time' --thetamax 180.000000 --spectralfiles 'no' --liketype 'unbinned' --optimizeposition 'no' --datarepository '.' --ltcube '' --expomap '' --ulphindex -2.000000 --flemin 100.000000 --flemax 10000.000000 --fgl_mode 'fast'
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 25.19240 FROM MIGRAD STATUS=CONVERGED 60 CALLS 61 TOTAL
EDM= .29E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 10.019 3.3143 .30809E-02 -.27813
2 Index -3.5319 .64720 .24212E-01 .32115E-01
3 Value .99981 .12972 .56233E-01 -.26450E-02
4 Normalizat 2.8054 6.2903 .45249 -.10892E-01
ERR DEF= .500
Final values:
Integral = 10.0191
Index = -3.53186
Value = 0.999814
Normalizat = 2.80535
**********
** 6 **HESSE
**********
FCN= 25.19240 FROM HESSE STATUS=OK 23 CALLS 84 TOTAL
EDM= .29E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 10.019 3.3051 .78916E-04 -1.3703
2 Index -3.5319 .64551 .10702E-03 -.17962
3 Value .99981 .12967 .12381E-02 -.61880E-03
4 Normalizat 2.8054 6.2903 .33759E-01 -.47065
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.000290278
Minuit parameter uncertainties:
1 3.3057
2 0.650748
3 0.134091
4 4.41192
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/MPLPlot.py:54: UserWarning: Matplotlib is currently using agg, which is a non-GUI backend, so cannot show the figure.
self.fig.show()
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/MPLPlot.py:65: UserWarning: Matplotlib is currently using agg, which is a non-GUI backend, so cannot show the figure.
self.fig.show()
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 13.71579 FROM MIGRAD STATUS=CONVERGED 59 CALLS 60 TOTAL
EDM= .58E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 26.952 8.8630 .30809E-02 .65340E-01
2 Index -3.7796 .70457 .20222E-01 .30755E-01
3 Value 1.0001 .12965 .41829E-01 .75755E-03
4 Normalizat 2.9582 6.3568 .45249 -.22647E-01
ERR DEF= .500
Final values:
Integral = 26.9515
Index = -3.77959
Value = 1.0001
Normalizat = 2.95819
**********
** 6 **HESSE
**********
FCN= 13.71579 FROM HESSE STATUS=OK 23 CALLS 83 TOTAL
EDM= .58E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 26.952 8.8450 .97062E-04 -1.2410
2 Index -3.7796 .70322 .89390E-04 -.26416
3 Value 1.0001 .12962 .92077E-03 .34741E-03
4 Normalizat 2.9582 6.3568 .18578E-01 -.43630
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00057519
Minuit parameter uncertainties:
1 8.84939
2 0.7103
3 0.134031
4 4.48722
Requested intervals:
------------------------------------------------------
2.6996 - 3.6358
3.6358 - 3.9968
3.9968 - 4.4024
4.4024 - 4.7375
4.7375 - 5.0909
5.0909 - 5.5471
5.5471 - 5.9896
5.9896 - 6.3998
6.3998 - 6.6889
6.6889 - 7.0117
7.0117 - 7.2936
7.2936 - 7.7731
7.7731 - 8.2167
8.2167 - 8.8763
8.8763 - 9.6573
9.6573 - 10.568
10.568 - 12.0568
12.0568 - 14.6165
14.6165 - 17.7834
17.7834 - 21.4962
21.4962 - 30.0798
30.0798 - 40.8747
40.8747 - 48.7118
48.7118 - 73.7262
73.7262 - 172.5754
Data files:
-----------
eventfile /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit
ft2file /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
rspfile /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp
cspecfile /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.pha
ROI:
-----
R.A. 54.51
Dec. -26.939
Radius 10.0
Interval # 1 (2.6996-3.6358):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_2.6996-3.6358.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='2.6996' tstop='3.6358' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192230.3256 tstop=569192231.2618 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192230.3256 tmax=569192231.2618 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_2.6996-3.6358.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.02
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.9362000226974487
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_2.6996-3.6358.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_2.6996-3.6358.xml 0.9362000226974487 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_2.6996-3.6358.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_2.6996-3.6358.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval2.6996-3.6358/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.97
user 0.37
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval2.6996-3.6358/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval2.6996-3.6358/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_2.6996-3.6358.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval2.6996-3.6358/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.50
user 8.04
sys 1.33
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval2.6996-3.6358/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_2.6996-3.6358.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.953494127561727
srcName 0.0011338410199896408
srcName 0.007606934309661652
Resid 10.0 9.962237479816439 -13.802931656814316
plotting GRB spectrum
srcName 9.953494127561727
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 93|
| | Integral| 0.01| 0.00331| ph./cm2/s| |
| | Index| -3.53| 0.651| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 2.65e-06| 8.62e-07| erg/cm2/s| |
| | Photon flux| 0.01| 0.00331| ph./cm2/s| |
|GalacticTemplate | | | | | 1|
| | Value| 1| 0.134| -| |
| | Energy flux| 3.76e-07| 5.04e-08| erg/cm2/s| |
| | Photon flux| 0.000519| 6.97e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 2.81| 4.41| -| |
| | Energy flux| 3.33e-07| 5.23e-07| erg/cm2/s| |
| | Photon flux| 0.000724| 0.00114| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 25.192404030402265
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval2.6996-3.6358/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval2.6996-3.6358/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.49
user 6.61
sys 0.73
Interval # 2 (3.6358-3.9968):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_3.6358-3.9968.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='3.6358' tstop='3.9968' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192231.2618 tstop=569192231.6228 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.10
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192231.2618 tmax=569192231.6228 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_3.6358-3.9968.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.3609999418258667
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_3.6358-3.9968.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_3.6358-3.9968.xml 0.3609999418258667 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_3.6358-3.9968.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_3.6358-3.9968.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.6358-3.9968/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.93
user 0.37
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.6358-3.9968/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Starting calculation of region 20.0,0.0 to 40.0,40.0
Completed calculation of region 20.0,0.0 to 40.0,40.0
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 4.786573 FROM MIGRAD STATUS=CONVERGED 59 CALLS 60 TOTAL
EDM= .14E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 21.180 7.0327 .23636E-02 -.13186E-01
2 Index -2.9699 .52925 .85627E-02 -.18188E-02
3 Value .99991 .14384 .25508E-01 -.11507E-02
4 Normalizat 1.1343 6.1424 .45249 .18243E-02
ERR DEF= .500
Final values:
Integral = 21.1798
Index = -2.96985
Value = 0.999907
Normalizat = 1.13433
**********
** 6 **HESSE
**********
FCN= 4.786573 FROM HESSE STATUS=OK 23 CALLS 83 TOTAL
EDM= .14E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 21.180 7.0233 .10446E-04 -1.2787
2 Index -2.9699 .52858 .37854E-04 .83682E-02
3 Value .99991 .14383 .56140E-03 -.30964E-03
4 Normalizat 1.1343 5.7403 .23309E-01 -.91251
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00141206
Minuit parameter uncertainties:
1 7.02613
2 0.531342
3 0.15
4 62.343
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 5.901543 FROM MIGRAD STATUS=CONVERGED 60 CALLS 61 TOTAL
EDM= .70E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 23.160 7.6988 .30809E-02 -.91845E-02
2 Index -2.4923 .42491 .76520E-02 .31986E-02
3 Value 1.0000 .14384 .28069E-01 .41330E-03
4 Normalizat .91020 5.1008 .45249 .10450E-02
ERR DEF= .500
Final values:
Integral = 23.1596
Index = -2.49229
Value = 1.00003
Normalizat = 0.910198
**********
** 6 **HESSE
**********
FCN= 5.901543 FROM HESSE STATUS=OK 23 CALLS 84 TOTAL
EDM= .69E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 23.160 7.6891 .12032E-04 -1.2652
2 Index -2.4923 .42439 .33820E-04 .16808
3 Value 1.0000 .14383 .61779E-03 .89776E-04
4 Normalizat .91020 5.0832 .31196E-01 -.99054
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.000686004
Minuit parameter uncertainties:
1 7.69242
2 0.425859
3 0.15
4 67.9551
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.6358-3.9968/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_3.6358-3.9968.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.6358-3.9968/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.39
user 7.78
sys 1.52
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.6358-3.9968/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_3.6358-3.9968.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.986960806902863
srcName 0.0004373373203917359
srcName 0.003093054675831681
Resid 10.0 9.990493775824152 -10.57745949602455
plotting GRB spectrum
srcName 9.986960806902863
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 120|
| | Integral| 0.027| 0.00885| ph./cm2/s| |
| | Index| -3.78| 0.71| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 6.75e-06| 2.16e-06| erg/cm2/s| |
| | Photon flux| 0.027| 0.00885| ph./cm2/s| |
|GalacticTemplate | | | | | 1|
| | Value| 1| 0.134| -| |
| | Energy flux| 3.76e-07| 5.04e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 6.96e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 2.96| 4.49| -| |
| | Energy flux| 3.51e-07| 5.32e-07| erg/cm2/s| |
| | Photon flux| 0.000763| 0.00116| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 13.71578628453528
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.6358-3.9968/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.6358-3.9968/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.60
user 6.12
sys 1.40
Interval # 3 (3.9968-4.4024):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_3.9968-4.4024.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='3.9968' tstop='4.4024' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192231.6228 tstop=569192232.0284001 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192231.6228 tmax=569192232.0284001 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_3.9968-4.4024.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.18
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.40560007095336914
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_3.9968-4.4024.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_3.9968-4.4024.xml 0.40560007095336914 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_3.9968-4.4024.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_3.9968-4.4024.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.9968-4.4024/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.89
user 0.36
sys 0.43
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.9968-4.4024/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.9968-4.4024/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_3.9968-4.4024.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.9968-4.4024/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.78
user 7.92
sys 1.79
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.9968-4.4024/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_3.9968-4.4024.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.996561405421195
srcName 0.0004912717898511938
srcName 0.0013325793304965982
Resid 10.0 9.998387833466605 -11.290687001616892
plotting GRB spectrum
srcName 9.996561405421195
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 141|
| | Integral| 0.0212| 0.00703| ph./cm2/s| |
| | Index| -2.97| 0.531| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 6.81e-06| 2.38e-06| erg/cm2/s| |
| | Photon flux| 0.0212| 0.00703| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 1.13| 62.3| -| |
| | Energy flux| 1.34e-07| 7.39e-06| erg/cm2/s| |
| | Photon flux| 0.000293| 0.0161| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 4.786573452308374
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.9968-4.4024/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval3.9968-4.4024/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.12
user 6.00
sys 1.08
Interval # 4 (4.4024-4.7375):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_4.4024-4.7375.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='4.4024' tstop='4.7375' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192232.0284001 tstop=569192232.3635 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.10
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192232.0284001 tmax=569192232.3635 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.13
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_4.4024-4.7375.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.18
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.3350999355316162
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 13.43105 FROM MIGRAD STATUS=CONVERGED 67 CALLS 68 TOTAL
EDM= .19E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 20.171 6.6684 .30809E-02 -.90907E-03
2 Index -2.1563 .36095 .98953E-02 -.29639E-02
3 Value .99998 .14387 .41408E-01 .17671E-03
4 Normalizat 1.3383 5.4857 .45249 .21185E-02
ERR DEF= .500
Final values:
Integral = 20.1712
Index = -2.15626
Value = 0.99998
Normalizat = 1.33826
**********
** 6 **HESSE
**********
FCN= 13.43105 FROM HESSE STATUS=OK 23 CALLS 91 TOTAL
EDM= .19E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 20.171 6.6627 .16539E-04 -1.2858
2 Index -2.1563 .36063 .43715E-04 .28287
3 Value .99998 .14383 .91150E-03 -3.1415
4 Normalizat 1.3383 5.1427 .37505E-01 -.84783
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00186985
Minuit parameter uncertainties:
1 6.66524
2 0.361579
3 0.15
4 66.8306
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
MIGRAD MINIMIZATION HAS CONVERGED.
FCN= 11.37565 FROM MIGRAD STATUS=CONVERGED 74 CALLS 75 TOTAL
EDM= .16E-05 STRATEGY=1 ERROR MATRIX UNCERTAINTY= 9.4%
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 12.383 4.1741 .46185E-04 .11183E-01
2 Index -1.3575 .28307 -.39655E-04 -.82376E-02
3 Value 1.0000 .14387 -.44493E-03 .59210E-03
4 Normalizat .10129 7.8813 -.88047 -.60995E-04
ERR DEF= .500
Final values:
Integral = 12.3829
Index = -1.35747
Value = 1.00004
Normalizat = 0.101295
**********
** 6 **HESSE
**********
FCN= 11.37565 FROM HESSE STATUS=OK 25 CALLS 100 TOTAL
EDM= .24E-05 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 12.383 4.1657 .12561E-04 -1.3478
2 Index -1.3575 .28245 .18725E-03 .57631
3 Value 1.0000 .14383 .84157E-03 .12584E-03
4 Normalizat .10129 5.4882 .40571 -1.5937
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 2.44346e-06
Minuit parameter uncertainties:
1 4.16671
2 0.283048
3 0.15
4 2.20749
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_4.4024-4.7375.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_4.4024-4.7375.xml 0.3350999355316162 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_4.4024-4.7375.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_4.4024-4.7375.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.4024-4.7375/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.91
user 0.38
sys 0.44
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.4024-4.7375/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.4024-4.7375/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_4.4024-4.7375.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.4024-4.7375/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.75
user 7.83
sys 1.85
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.4024-4.7375/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_4.4024-4.7375.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.99788868273325
srcName 0.00040592912100504845
srcName 0.0008834133534375847
Resid 10.0 9.999180602132755 -4.61811626925867
plotting GRB spectrum
srcName 9.99788868273325
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 147|
| | Integral| 0.0232| 0.00769| ph./cm2/s| |
| | Index| -2.49| 0.426| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.01e-05| 4.08e-06| erg/cm2/s| |
| | Photon flux| 0.0231| 0.0077| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.91| 68| -| |
| | Energy flux| 1.08e-07| 8.06e-06| erg/cm2/s| |
| | Photon flux| 0.000235| 0.0175| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 5.901542808986707
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.4024-4.7375/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.4024-4.7375/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.25
user 6.39
sys 0.84
Interval # 5 (4.7375-5.0909):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_4.7375-5.0909.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='4.7375' tstop='5.0909' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192232.3635 tstop=569192232.7169 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192232.3635 tmax=569192232.7169 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_4.7375-5.0909.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.14
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.35339999198913574
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_4.7375-5.0909.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_4.7375-5.0909.xml 0.35339999198913574 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_4.7375-5.0909.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_4.7375-5.0909.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.7375-5.0909/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.95
user 0.36
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.7375-5.0909/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Starting calculation of region 20.0,0.0 to 40.0,40.0
Completed calculation of region 20.0,0.0 to 40.0,40.0
Starting calculation of region 0.0,0.0 to 20.0,40.0
Completed calculation of region 0.0,0.0 to 20.0,40.0
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.7375-5.0909/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_4.7375-5.0909.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.7375-5.0909/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.34
user 7.64
sys 1.63
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.7375-5.0909/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_4.7375-5.0909.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.999499601091127
srcName 0.00042807703921249747
srcName 0.001369811575685584
Resid 10.0 10.00130006663109 4.3116585425461444
plotting GRB spectrum
srcName 9.999499601091127
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 145|
| | Integral| 0.0202| 0.00667| ph./cm2/s| |
| | Index| -2.16| 0.362| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.23e-05| 5.57e-06| erg/cm2/s| |
| | Photon flux| 0.0201| 0.00668| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 1.34| 66.8| -| |
| | Energy flux| 1.59e-07| 7.92e-06| erg/cm2/s| |
| | Photon flux| 0.000345| 0.0172| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 13.431052285715046
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.7375-5.0909/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval4.7375-5.0909/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.31
user 5.97
sys 1.30
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
MIGRAD MINIMIZATION HAS CONVERGED.
FCN= 7.632503 FROM MIGRAD STATUS=CONVERGED 61 CALLS 62 TOTAL
EDM= .99E-06 STRATEGY=1 ERROR MATRIX UNCERTAINTY= 5.3%
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 15.976 5.2757 -.11292E-05 .49973E-02
2 Index -2.1244 .35547 .61855E-04 -.11320E-02
3 Value .99998 .14385 .21549E-03 -.15442E-03
4 Normalizat .10078 9.7186 -.69886 -.81697E-04
ERR DEF= .500
Final values:
Integral = 15.9761
Index = -2.12439
Value = 0.999979
Normalizat = 0.100778
**********
** 6 **HESSE
**********
FCN= 7.632503 FROM HESSE STATUS=OK 25 CALLS 87 TOTAL
EDM= .15E-05 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 15.976 5.2715 .11222E-04 -1.3173
2 Index -2.1244 .35516 .33038E-04 .29394
3 Value .99998 .14383 .69639E-03 -.70079E-04
4 Normalizat .10078 8.9152 .23472 -1.5885
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 1.54222e-06
Minuit parameter uncertainties:
1 5.2731
2 0.356067
3 0.15
4 1.29574
Interval # 6 (5.0909-5.5471):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_5.0909-5.5471.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='5.0909' tstop='5.5471' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192232.7169 tstop=569192233.1731 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192232.7169 tmax=569192233.1731 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 9 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_5.0909-5.5471.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 9
Total time in Good Time Intervals: 0.4562000036239624
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_5.0909-5.5471.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_5.0909-5.5471.xml 0.4562000036239624 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_5.0909-5.5471.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_5.0909-5.5471.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.0909-5.5471/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.89
user 0.36
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.0909-5.5471/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.0909-5.5471/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_5.0909-5.5471.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.0909-5.5471/gll_ft1_tr_bn190114873_v00_filt.fit.........!
real 10.60
user 8.80
sys 1.74
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.0909-5.5471/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_5.0909-5.5471.xml
Optimizer: Minuit
Performing likelihood fit...
Data 9.0
srcName 2.576925063095601e-06
srcName 9.001051106105008
srcName 0.0005526317380483205
srcName 0.00013384314356251235
Resid 9.0 9.001740157911682 -2.0136879590350185
plotting GRB spectrum
srcName 9.001051106105008
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 163|
| | Integral| 0.0124| 0.00417| ph./cm2/s| |
| | Index| -1.36| 0.283| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 2.2e-05| 1.1e-05| erg/cm2/s| |
| | Photon flux| 0.0109| 0.00376| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.101| 2.21| -| |
| | Energy flux| 1.2e-08| 2.62e-07| erg/cm2/s| |
| | Photon flux| 2.61e-05| 0.000569| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 11.375651148462001
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.0909-5.5471/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.0909-5.5471/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.37
user 6.19
sys 1.14
Interval # 7 (5.5471-5.9896):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_5.5471-5.9896.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='5.5471' tstop='5.9896' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192233.1731 tstop=569192233.6156 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.10
user 0.05
sys 0.04
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192233.1731 tmax=569192233.6156 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.13
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_5.5471-5.9896.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.14
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.4424999952316284
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_5.5471-5.9896.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_5.5471-5.9896.xml 0.4424999952316284 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_5.5471-5.9896.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_5.5471-5.9896.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.5471-5.9896/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.90
user 0.37
sys 0.44
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.5471-5.9896/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.5471-5.9896/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_5.5471-5.9896.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 10.79486 FROM MIGRAD STATUS=CONVERGED 60 CALLS 61 TOTAL
EDM= .15E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 19.021 6.3293 .30809E-02 -.66619E-01
2 Index -2.5185 .43048 .10279E-01 -.15780E-01
3 Value 1.0003 .14386 .37285E-01 .41740E-02
4 Normalizat 1.6066 5.4634 .45249 .14402E-02
ERR DEF= .500
Final values:
Integral = 19.0206
Index = -2.51846
Value = 1.00031
Normalizat = 1.60661
**********
** 6 **HESSE
**********
FCN= 10.79486 FROM HESSE STATUS=OK 23 CALLS 84 TOTAL
EDM= .15E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 19.021 6.3190 .72286E-04 -1.2941
2 Index -2.5185 .42982 .45431E-04 .15926
3 Value 1.0003 .14383 .82069E-03 .10274E-02
4 Normalizat 1.6066 5.0019 .44279E-01 -.76930
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00150618
Minuit parameter uncertainties:
1 6.32126
2 0.431336
3 0.15
4 95.1762
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 6.844639 FROM MIGRAD STATUS=CONVERGED 66 CALLS 67 TOTAL
EDM= .31E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 25.622 7.9899 .30809E-02 -.59727E-02
2 Index -1.9400 .31092 .64137E-02 -.13102E-02
3 Value .99998 .14385 .30066E-01 -.21064E-03
4 Normalizat .43639 9.0739 .45249 -.79033E-03
ERR DEF= .500
Final values:
Integral = 25.6224
Index = -1.94
Value = 0.99998
Normalizat = 0.436387
**********
** 6 **HESSE
**********
FCN= 6.844639 FROM HESSE STATUS=OK 23 CALLS 90 TOTAL
EDM= .31E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 25.622 7.9910 .12940E-04 -8.1755
2 Index -1.9400 .31095 .28323E-04 -3.5003
3 Value .99998 .14383 .66175E-03 -.68041E-04
4 Normalizat .43639 9.3573 .29597E-01 -1.9416
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00030737
Minuit parameter uncertainties:
1 7.99439
2 0.311586
3 0.15
4 39.7783
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.5471-5.9896/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.28
user 7.49
sys 1.74
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.5471-5.9896/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_5.5471-5.9896.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 10.000748366300273
srcName 0.0005360043373690395
srcName 0.00012916130993859034
Resid 10.0 10.001416108872645 -7.223755283655143
plotting GRB spectrum
srcName 10.000748366300273
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 154|
| | Integral| 0.016| 0.00527| ph./cm2/s| |
| | Index| -2.12| 0.356| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.01e-05| 4.63e-06| erg/cm2/s| |
| | Photon flux| 0.0159| 0.00528| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.101| 1.3| -| |
| | Energy flux| 1.19e-08| 1.54e-07| erg/cm2/s| |
| | Photon flux| 2.6e-05| 0.000334| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 7.632502730875872
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.5471-5.9896/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.5471-5.9896/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.11
user 5.78
sys 1.26
Interval # 8 (5.9896-6.3998):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_5.9896-6.3998.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='5.9896' tstop='6.3998' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192233.6156 tstop=569192234.0258 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192233.6156 tmax=569192234.0258 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_5.9896-6.3998.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.41019999980926514
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_5.9896-6.3998.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_5.9896-6.3998.xml 0.41019999980926514 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_5.9896-6.3998.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_5.9896-6.3998.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.9896-6.3998/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.91
user 0.37
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.9896-6.3998/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.9896-6.3998/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_5.9896-6.3998.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.9896-6.3998/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.26
user 7.68
sys 1.53
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.9896-6.3998/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_5.9896-6.3998.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.989220296403241
srcName 0.0004970426397547866
srcName 0.0019087962756604146
Resid 10.0 9.99162871224372 -7.09976154984337
plotting GRB spectrum
srcName 9.989220296403241
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 138|
| | Integral| 0.019| 0.00632| ph./cm2/s| |
| | Index| -2.52| 0.431| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 8.11e-06| 3.25e-06| erg/cm2/s| |
| | Photon flux| 0.019| 0.00633| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 1.61| 95.2| -| |
| | Energy flux| 1.9e-07| 1.13e-05| erg/cm2/s| |
| | Photon flux| 0.000414| 0.0245| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 10.794860775261109
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.9896-6.3998/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval5.9896-6.3998/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 6.69
user 5.77
sys 0.88
Interval # 9 (6.3998-6.6889):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_6.3998-6.6889.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='6.3998' tstop='6.6889' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192234.0258 tstop=569192234.3149 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192234.0258 tmax=569192234.3149 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.11
user 0.08
sys 0.02
Selected 11 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_6.3998-6.6889.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 11
Total time in Good Time Intervals: 0.2891000509262085
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_6.3998-6.6889.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_6.3998-6.6889.xml 0.2891000509262085 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 8.317516 FROM MIGRAD STATUS=CONVERGED 55 CALLS 56 TOTAL
EDM= .68E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 20.396 7.1130 .30809E-02 -.56667E-01
2 Index -2.2587 .39603 .86166E-02 .27737E-01
3 Value 1.0010 .12975 .32943E-01 .13867E-01
4 Normalizat 1.0222 5.2348 .45249 -.51949E-03
ERR DEF= .500
Final values:
Integral = 20.396
Index = -2.25873
Value = 1.00104
Normalizat = 1.02216
**********
** 6 **HESSE
**********
FCN= 8.317516 FROM HESSE STATUS=OK 23 CALLS 79 TOTAL
EDM= .67E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 20.396 7.1060 .69765E-04 -1.2842
2 Index -2.2587 .39563 .38072E-04 .24754
3 Value 1.0010 .12973 .72510E-03 .34687E-02
4 Normalizat 1.0222 5.2348 .54398E-01 -.95050
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 6.74581e-05
Minuit parameter uncertainties:
1 7.10897
2 0.396855
3 0.134155
4 2.87733
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 12.58093 FROM MIGRAD STATUS=CONVERGED 62 CALLS 63 TOTAL
EDM= .10E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 23.503 7.6489 .30809E-02 .23418E-02
2 Index -1.8763 .31680 .88443E-02 -.13374E-02
3 Value 1.00000 .14386 .40124E-01 .17968E-04
4 Normalizat .90688 6.4733 .45249 .15404E-02
ERR DEF= .500
Final values:
Integral = 23.5034
Index = -1.87628
Value = 0.999996
Normalizat = 0.906883
**********
** 6 **HESSE
**********
FCN= 12.58093 FROM HESSE STATUS=OK 23 CALLS 86 TOTAL
EDM= .10E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 23.503 7.6555 .17329E-04 -1.8786
2 Index -1.8763 .31706 .39054E-04 .38147
3 Value 1.00000 .14383 .88323E-03 -.13533E-04
4 Normalizat .90688 6.0597 .36689E-01 -.99177
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00100744
Minuit parameter uncertainties:
1 7.65875
2 0.317742
3 0.15
4 55.7999
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/MPLPlot.py:41: RuntimeWarning: More than 20 figures have been opened. Figures created through the pyplot interface (`matplotlib.pyplot.figure`) are retained until explicitly closed and may consume too much memory. (To control this warning, see the rcParam `figure.max_open_warning`). Consider using `matplotlib.pyplot.close()`.
self.fig = plt.figure()
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_6.3998-6.6889.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_6.3998-6.6889.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.3998-6.6889/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.87
user 0.35
sys 0.43
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.3998-6.6889/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.3998-6.6889/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_6.3998-6.6889.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.3998-6.6889/gll_ft1_tr_bn190114873_v00_filt.fit...........!
real 9.09
user 7.49
sys 1.55
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.3998-6.6889/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_6.3998-6.6889.xml
Optimizer: Minuit
Performing likelihood fit...
Data 11.0
srcName 2.576925063095601e-06
srcName 11.000959917900444
srcName 0.0003501897711009747
srcName 0.00036540428798170603
Resid 11.0 11.00167808888459 1.3802163605436135
plotting GRB spectrum
srcName 11.000959917900444
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 184|
| | Integral| 0.0256| 0.00799| ph./cm2/s| |
| | Index| -1.94| 0.312| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 2.05e-05| 9.35e-06| erg/cm2/s| |
| | Photon flux| 0.0253| 0.00801| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.436| 39.8| -| |
| | Energy flux| 5.17e-08| 4.72e-06| erg/cm2/s| |
| | Photon flux| 0.000113| 0.0103| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 6.844638634332356
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.3998-6.6889/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.3998-6.6889/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.12
user 6.07
sys 1.00
Interval # 10 (6.6889-7.0117):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_6.6889-7.0117.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='6.6889' tstop='7.0117' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192234.3149 tstop=569192234.6377001 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192234.3149 tmax=569192234.6377001 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 9 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_6.6889-7.0117.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 9
Total time in Good Time Intervals: 0.32280004024505615
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_6.6889-7.0117.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_6.6889-7.0117.xml 0.32280004024505615 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_6.6889-7.0117.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_6.6889-7.0117.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.6889-7.0117/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.94
user 0.36
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.6889-7.0117/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.6889-7.0117/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_6.6889-7.0117.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.6889-7.0117/gll_ft1_tr_bn190114873_v00_filt.fit.........!
real 9.89
user 7.88
sys 1.96
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.6889-7.0117/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_6.6889-7.0117.xml
Optimizer: Minuit
Performing likelihood fit...
Data 9.0
srcName 2.576925063095601e-06
srcName 8.990461521369793
srcName 0.00039142577778120884
srcName 0.0009556676163011872
Resid 9.0 8.991811191688937 -4.7815117536717535
plotting GRB spectrum
srcName 8.990461521369793
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 131|
| | Integral| 0.0204| 0.00711| ph./cm2/s| |
| | Index| -2.26| 0.397| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.11e-05| 5.11e-06| erg/cm2/s| |
| | Photon flux| 0.0203| 0.00712| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.134| -| |
| | Energy flux| 3.76e-07| 5.05e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 6.97e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 1.02| 2.88| -| |
| | Energy flux| 1.21e-07| 3.41e-07| erg/cm2/s| |
| | Photon flux| 0.000264| 0.000742| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 8.317516026690823
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.6889-7.0117/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval6.6889-7.0117/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.34
user 6.34
sys 0.96
Interval # 11 (7.0117-7.2936):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_7.0117-7.2936.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='7.0117' tstop='7.2936' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192234.6377001 tstop=569192234.9196 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 18.30164 FROM MIGRAD STATUS=CONVERGED 68 CALLS 69 TOTAL
EDM= .14E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 13.620 4.4223 .30809E-02 -.12540E-01
2 Index -1.8169 .30959 .10480E-01 .16217E-02
3 Value .99996 .14388 .48105E-01 -.40319E-03
4 Normalizat .18778 9.0763 .45249 -.72743E-03
ERR DEF= .500
Final values:
Integral = 13.6204
Index = -1.81695
Value = 0.999961
Normalizat = 0.187781
**********
** 6 **HESSE
**********
FCN= 18.30164 FROM HESSE STATUS=OK 23 CALLS 92 TOTAL
EDM= .14E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 13.620 4.4172 .15736E-04 -7.6200
2 Index -1.8169 .30921 .46275E-04 -3.5444
3 Value .99996 .14383 .10590E-02 -.12931E-03
4 Normalizat .18778 9.3081 .34586E-01 -1.7594
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.000139175
Minuit parameter uncertainties:
1 4.41827
2 0.309854
3 0.15
4 15.0328
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192234.6377001 tmax=569192234.9196 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_7.0117-7.2936.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.28189992904663086
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_7.0117-7.2936.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_7.0117-7.2936.xml 0.28189992904663086 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_7.0117-7.2936.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_7.0117-7.2936.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.0117-7.2936/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.94
user 0.36
sys 0.43
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.0117-7.2936/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.0117-7.2936/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_7.0117-7.2936.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.0117-7.2936/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 9.03
user 7.70
sys 1.29
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.0117-7.2936/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_7.0117-7.2936.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.999589186527665
srcName 0.000341473770137722
srcName 0.0007404571213157646
Resid 10.0 10.00067369434418 -2.828334300941889
plotting GRB spectrum
srcName 9.999589186527665
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 156|
| | Integral| 0.0235| 0.00766| ph./cm2/s| |
| | Index| -1.88| 0.318| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 2.05e-05| 1.25e-05| erg/cm2/s| |
| | Photon flux| 0.0231| 0.00744| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.907| 55.8| -| |
| | Energy flux| 1.08e-07| 6.62e-06| erg/cm2/s| |
| | Photon flux| 0.000234| 0.0144| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 12.580930794139656
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.0117-7.2936/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.0117-7.2936/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 6.93
user 6.13
sys 0.77
Interval # 12 (7.2936-7.7731):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_7.2936-7.7731.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='7.2936' tstop='7.7731' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192234.9196 tstop=569192235.3991001 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192234.9196 tmax=569192235.3991001 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.11
user 0.08
sys 0.02
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_7.2936-7.7731.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.02
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.47950005531311035
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_7.2936-7.7731.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_7.2936-7.7731.xml 0.47950005531311035 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_7.2936-7.7731.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_7.2936-7.7731.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.2936-7.7731/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.98
user 0.39
sys 0.46
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.2936-7.7731/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.2936-7.7731/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_7.2936-7.7731.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.2936-7.7731/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 8.17
user 7.38
sys 0.75
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.2936-7.7731/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_7.2936-7.7731.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.998483483004073
srcName 0.0005808125234028571
srcName 0.00026079203083161827
Resid 10.0 9.999327664483369 1.1622207672024185
plotting GRB spectrum
srcName 9.998483483004073
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 14.90094 FROM MIGRAD STATUS=CONVERGED 59 CALLS 60 TOTAL
EDM= .44E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 18.001 5.9793 .30809E-02 -.25800E-01
2 Index -2.6182 .44644 .12529E-01 .35049E-02
3 Value 1.0001 .12966 .43537E-01 .75805E-03
4 Normalizat 1.0080 5.2231 .45249 -.65000E-02
ERR DEF= .500
Final values:
Integral = 18.0009
Index = -2.6182
Value = 1.00008
Normalizat = 1.008
**********
** 6 **HESSE
**********
FCN= 14.90094 FROM HESSE STATUS=OK 23 CALLS 83 TOTAL
EDM= .44E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 18.001 5.9685 .16418E-04 -1.3017
2 Index -2.6182 .44564 .55378E-04 .12572
3 Value 1.0001 .12963 .95841E-03 .25507E-03
4 Normalizat 1.0080 5.2232 .20209E-01 -.95544
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 4.42951e-05
Minuit parameter uncertainties:
1 5.97049
2 0.447312
3 0.134042
4 2.85741
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
MIGRAD MINIMIZATION HAS CONVERGED.
FCN= 13.18701 FROM MIGRAD STATUS=CONVERGED 62 CALLS 63 TOTAL
EDM= .24E-05 STRATEGY=1 ERROR MATRIX UNCERTAINTY= 6.5%
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 10.844 3.5878 .22435E-04 .17397E-01
2 Index -2.1681 .36364 .28080E-03 -.86890E-02
3 Value .99991 .14390 .11682E-02 -.10236E-02
4 Normalizat .10118 7.3526 -.76552 -.80068E-04
ERR DEF= .500
Final values:
Integral = 10.8436
Index = -2.16813
Value = 0.999914
Normalizat = 0.101181
**********
** 6 **HESSE
**********
FCN= 13.18701 FROM HESSE STATUS=OK 25 CALLS 88 TOTAL
EDM= .40E-05 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 10.844 3.5833 .11964E-04 -1.3622
2 Index -2.1681 .36268 .43529E-04 .27876
3 Value .99991 .14383 .90351E-03 -.28698E-03
4 Normalizat .10118 8.9261 .35041 -1.5926
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 3.99092e-06
Minuit parameter uncertainties:
1 3.58406
2 0.363643
3 0.15
4 1.79574
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 152|
| | Integral| 0.0136| 0.00442| ph./cm2/s| |
| | Index| -1.82| 0.31| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.29e-05| 7.79e-06| erg/cm2/s| |
| | Photon flux| 0.0134| 0.00427| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.188| 15| -| |
| | Energy flux| 2.23e-08| 1.78e-06| erg/cm2/s| |
| | Photon flux| 4.84e-05| 0.00388| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 18.3016350065737
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.2936-7.7731/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.2936-7.7731/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 6.92
user 5.94
sys 0.89
Interval # 13 (7.7731-8.2167):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_7.7731-8.2167.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='7.7731' tstop='8.2167' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192235.3991001 tstop=569192235.8427 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192235.3991001 tmax=569192235.8427 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_7.7731-8.2167.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.21
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.4435999393463135
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_7.7731-8.2167.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_7.7731-8.2167.xml 0.4435999393463135 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_7.7731-8.2167.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_7.7731-8.2167.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.7731-8.2167/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.98
user 0.37
sys 0.44
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.7731-8.2167/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.7731-8.2167/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_7.7731-8.2167.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.7731-8.2167/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 10.48
user 9.07
sys 1.31
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.7731-8.2167/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_7.7731-8.2167.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.991435037273748
srcName 0.0005373890998907943
srcName 0.001295102495891409
Resid 10.0 9.993270105794592 -6.909179893973825
plotting GRB spectrum
srcName 9.991435037273748
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 128|
| | Integral| 0.018| 0.00597| ph./cm2/s| |
| | Index| -2.62| 0.447| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 7.11e-06| 2.74e-06| erg/cm2/s| |
| | Photon flux| 0.018| 0.00597| ph./cm2/s| |
|GalacticTemplate | | | | | 1|
| | Value| 1| 0.134| -| |
| | Energy flux| 3.76e-07| 5.04e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 6.96e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 1.01| 2.86| -| |
| | Energy flux| 1.2e-07| 3.39e-07| erg/cm2/s| |
| | Photon flux| 0.00026| 0.000737| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 14.900938117453087
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.7731-8.2167/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval7.7731-8.2167/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 6.80
user 6.04
sys 0.72
Interval # 14 (8.2167-8.8763):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_8.2167-8.8763.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='8.2167' tstop='8.8763' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192235.8427 tstop=569192236.5023 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.10
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192235.8427 tmax=569192236.5023 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_8.2167-8.8763.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.659600019454956
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_8.2167-8.8763.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_8.2167-8.8763.xml 0.659600019454956 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_8.2167-8.8763.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_8.2167-8.8763.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.2167-8.8763/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.95
user 0.36
sys 0.44
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 24.59086 FROM MIGRAD STATUS=CONVERGED 57 CALLS 58 TOTAL
EDM= .13E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 10.094 3.1842 .30809E-02 .14539
2 Index -2.1747 .34527 .12754E-01 .38583E-01
3 Value .99955 .12969 .55571E-01 -.61239E-02
4 Normalizat 1.7274 5.7300 .45249 -.95232E-02
ERR DEF= .500
Final values:
Integral = 10.0944
Index = -2.17472
Value = 0.999555
Normalizat = 1.72737
**********
** 6 **HESSE
**********
FCN= 24.59086 FROM HESSE STATUS=OK 23 CALLS 81 TOTAL
EDM= .13E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 10.094 3.1804 .14902E-04 -1.3695
2 Index -2.1747 .34484 .56346E-04 .27648
3 Value .99955 .12963 .12236E-02 -.14839E-02
4 Normalizat 1.7274 5.7300 .26867E-01 -.73588
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.000128655
Minuit parameter uncertainties:
1 3.18096
2 0.345663
3 0.134051
4 3.66924
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 28.24928 FROM MIGRAD STATUS=CONVERGED 56 CALLS 57 TOTAL
EDM= .18E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 6.9950 2.2560 .30809E-02 -.28481
2 Index -1.7279 .29675 .12808E-01 .29370E-02
3 Value 1.0000 .12939 .59484E-01 -.13854E-02
4 Normalizat 1.8401 5.7976 .45249 -.41803E-01
ERR DEF= .500
Final values:
Integral = 6.99502
Index = -1.72789
Value = 1.00004
Normalizat = 1.84009
**********
** 6 **HESSE
**********
FCN= 28.24928 FROM HESSE STATUS=OK 23 CALLS 80 TOTAL
EDM= .18E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 6.9950 2.2584 .69752E-04 -1.4033
2 Index -1.7279 .29703 .28279E-03 .43528
3 Value 1.0000 .12933 .13098E-02 .12951E-03
4 Normalizat 1.8401 5.7976 .14328E-01 -.70557
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00179872
Minuit parameter uncertainties:
1 2.25871
2 0.297622
3 0.133711
4 3.76865
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.2167-8.8763/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.2167-8.8763/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_8.2167-8.8763.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.2167-8.8763/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 8.77
user 7.59
sys 1.14
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.2167-8.8763/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_8.2167-8.8763.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 10.001570281304557
srcName 0.0007989275924652677
srcName 0.0001933016618915974
Resid 10.0 10.002565087483976 28.126986417375953
plotting GRB spectrum
srcName 10.001570281304557
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 146|
| | Integral| 0.0108| 0.00358| ph./cm2/s| |
| | Index| -2.17| 0.364| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 6.51e-06| 2.94e-06| erg/cm2/s| |
| | Photon flux| 0.0108| 0.00359| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.101| 1.8| -| |
| | Energy flux| 1.2e-08| 2.13e-07| erg/cm2/s| |
| | Photon flux| 2.61e-05| 0.000463| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 13.187014690229926
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.2167-8.8763/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.2167-8.8763/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.23
user 6.31
sys 0.87
Interval # 15 (8.8763-9.6573):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_8.8763-9.6573.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='8.8763' tstop='9.6573' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192236.5023 tstop=569192237.2833 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.10
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192236.5023 tmax=569192237.2833 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.02
Selected 11 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_8.8763-9.6573.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.02
Total number of events in the counts map: 11
Total time in Good Time Intervals: 0.781000018119812
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_8.8763-9.6573.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_8.8763-9.6573.xml 0.781000018119812 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_8.8763-9.6573.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_8.8763-9.6573.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.8763-9.6573/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.93
user 0.36
sys 0.44
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.8763-9.6573/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.8763-9.6573/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_8.8763-9.6573.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.8763-9.6573/gll_ft1_tr_bn190114873_v00_filt.fit...........!
real 8.83
user 7.78
sys 0.97
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.8763-9.6573/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_8.8763-9.6573.xml
Optimizer: Minuit
Performing likelihood fit...
Data 11.0
srcName 2.576925063095601e-06
srcName 11.00499239803732
srcName 0.0009456312301505176
srcName 0.003907426890059071
Resid 11.0 11.009848033082593 -4.8937666293935855
plotting GRB spectrum
srcName 11.00499239803732
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 136|
| | Integral| 0.0101| 0.00318| ph./cm2/s| |
| | Index| -2.17| 0.346| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 6.01e-06| 2.58e-06| erg/cm2/s| |
| | Photon flux| 0.0101| 0.00319| ph./cm2/s| |
|GalacticTemplate | | | | | 1|
| | Value| 1| 0.134| -| |
| | Energy flux| 3.76e-07| 5.04e-08| erg/cm2/s| |
| | Photon flux| 0.000519| 6.96e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 1.73| 3.67| -| |
| | Energy flux| 2.05e-07| 4.35e-07| erg/cm2/s| |
| | Photon flux| 0.000446| 0.000946| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 24.590861008360744
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.8763-9.6573/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval8.8763-9.6573/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.32
user 6.39
sys 0.88
Interval # 16 (9.6573-10.568):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_9.6573-10.568.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='9.6573' tstop='10.568' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192237.2833 tstop=569192238.194 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.11
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192237.2833 tmax=569192238.194 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.13
user 0.09
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_9.6573-10.568.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.18
user 0.14
sys 0.03
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 29.59265 FROM MIGRAD STATUS=CONVERGED 73 CALLS 74 TOTAL
EDM= .12E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 4.1402 1.3146 .30809E-02 -1.0157
2 Index -1.4685 .27324 .12885E-01 .34140E-01
3 Value 1.0007 .12956 .60858E-01 .88687E-02
4 Normalizat 1.9935 5.8856 .45249 -.27376E-01
ERR DEF= .500
Final values:
Integral = 4.14017
Index = -1.46846
Value = 1.00069
Normalizat = 1.99348
**********
** 6 **HESSE
**********
FCN= 29.59265 FROM HESSE STATUS=OK 23 CALLS 97 TOTAL
EDM= .12E-02 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 4.1402 1.3145 .54840E-04 -1.4420
2 Index -1.4685 .27322 .28483E-03 2.6087
3 Value 1.0007 .12950 .13401E-02 .23111E-02
4 Normalizat 1.9935 5.8856 .19216E-01 5.6177
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.00119924
Minuit parameter uncertainties:
1 1.31458
2 0.273727
3 0.133901
4 3.89468
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
MIGRAD MINIMIZATION HAS CONVERGED.
FCN= 30.55516 FROM MIGRAD STATUS=CONVERGED 60 CALLS 61 TOTAL
EDM= .11E-04 STRATEGY=1 ERROR MATRIX UNCERTAINTY= 6.1%
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 2.7185 .95514 .36492E-04 .16176
2 Index -2.4728 .44594 .11010E-02 -.10244E-01
3 Value 1.0000 .14392 -.78992E-03 .63655E-03
4 Normalizat .10104 9.6930 -.74347 -.23221E-03
ERR DEF= .500
Final values:
Integral = 2.71847
Index = -2.47282
Value = 1.00002
Normalizat = 0.101044
**********
** 6 **HESSE
**********
FCN= 30.55516 FROM HESSE STATUS=OK 25 CALLS 86 TOTAL
EDM= .19E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 2.7185 .95159 .94765E-05 -1.4665
2 Index -2.4728 .44303 .78024E-04 .17466
3 Value 1.0000 .14383 .13615E-02 .64687E-04
4 Normalizat .10104 9.8979 .29703 -1.5913
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 1.89434e-05
Minuit parameter uncertainties:
1 0.951645
2 0.444698
3 0.15
4 0.959761
Total number of events in the counts map: 10
Total time in Good Time Intervals: 0.9106999635696411
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_9.6573-10.568.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_9.6573-10.568.xml 0.9106999635696411 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_9.6573-10.568.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_9.6573-10.568.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval9.6573-10.568/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.96
user 0.37
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval9.6573-10.568/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval9.6573-10.568/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_9.6573-10.568.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval9.6573-10.568/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 8.60
user 7.56
sys 0.98
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval9.6573-10.568/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_9.6573-10.568.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.943634320737335
srcName 0.0011032053217912197
srcName 0.004853657610728121
Resid 10.0 9.94959376059492 -1.8601146034476042
plotting GRB spectrum
srcName 9.943634320737335
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 130|
| | Integral| 0.007| 0.00226| ph./cm2/s| |
| | Index| -1.73| 0.298| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 7.55e-06| 3.68e-06| erg/cm2/s| |
| | Photon flux| 0.0068| 0.00225| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.134| -| |
| | Energy flux| 3.76e-07| 5.03e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 6.95e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 1.84| 3.77| -| |
| | Energy flux| 2.18e-07| 4.47e-07| erg/cm2/s| |
| | Photon flux| 0.000475| 0.000972| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 28.249281387735333
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval9.6573-10.568/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval9.6573-10.568/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 8.38
user 7.59
sys 0.73
Interval # 17 (10.568-12.0568):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_10.568-12.0568.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='10.568' tstop='12.0568' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192238.194 tstop=569192239.6828 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192238.194 tmax=569192239.6828 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_10.568-12.0568.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.18
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 1.488800048828125
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_10.568-12.0568.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_10.568-12.0568.xml 1.488800048828125 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_10.568-12.0568.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_10.568-12.0568.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval10.568-12.0568/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.94
user 0.37
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval10.568-12.0568/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval10.568-12.0568/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_10.568-12.0568.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval10.568-12.0568/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 8.68
user 7.58
sys 1.02
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval10.568-12.0568/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_10.568-12.0568.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 9.908951061804515
srcName 0.0018046854663908737
srcName 0.008596113611400065
Resid 10.0 9.91935443780737 0.17787975762082375
plotting GRB spectrum
srcName 9.908951061804515
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 145|
| | Integral| 0.00414| 0.00131| ph./cm2/s| |
| | Index| -1.47| 0.274| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 6.43e-06| 3.07e-06| erg/cm2/s| |
| | Photon flux| 0.00381| 0.00126| ph./cm2/s| |
|GalacticTemplate | | | | | 1|
| | Value| 1| 0.134| -| |
| | Energy flux| 3.76e-07| 5.04e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 6.96e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 1.99| 3.89| -| |
| | Energy flux| 2.36e-07| 4.62e-07| erg/cm2/s| |
| | Photon flux| 0.000514| 0.001| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 29.59264898613047
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval10.568-12.0568/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval10.568-12.0568/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.58
user 6.60
sys 0.89
Interval # 18 (12.0568-14.6165):
-----------------------
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
MIGRAD MINIMIZATION HAS CONVERGED.
FCN= 29.31981 FROM MIGRAD STATUS=CONVERGED 55 CALLS 56 TOTAL
EDM= .64E-05 STRATEGY=1 ERROR MATRIX UNCERTAINTY= 3.9%
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 2.0480 .66040 .94538E-04 .17619
2 Index -1.7833 .30368 -.13400E-02 -.12302E-01
3 Value .99997 .14391 -.25868E-03 .14721E-03
4 Normalizat .10028 9.1390 -.62163 -.15151E-03
ERR DEF= .500
Final values:
Integral = 2.04801
Index = -1.7833
Value = 0.999966
Normalizat = 0.100277
**********
** 6 **HESSE
**********
FCN= 29.31981 FROM HESSE STATUS=OK 25 CALLS 81 TOTAL
EDM= .12E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 2.0480 .66251 .76375E-05 -1.4803
2 Index -1.7833 .30511 .28988E-03 .41504
3 Value .99997 .14383 .13341E-02 -.11179E-03
4 Normalizat .10028 8.6831 .24584 -1.5814
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 1.17459e-05
Minuit parameter uncertainties:
1 0.662534
2 0.30574
3 0.15
4 0.438866
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_12.0568-14.6165.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='12.0568' tstop='14.6165' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192239.6828 tstop=569192242.2425001 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.10
user 0.05
sys 0.04
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192239.6828 tmax=569192242.2425001 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.13
user 0.09
sys 0.03
Selected 9 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_12.0568-14.6165.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.23
user 0.16
sys 0.05
Total number of events in the counts map: 9
Total time in Good Time Intervals: 2.5597000122070312
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_12.0568-14.6165.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_12.0568-14.6165.xml 2.5597000122070312 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_12.0568-14.6165.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_12.0568-14.6165.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval12.0568-14.6165/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 1.00
user 0.37
sys 0.51
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval12.0568-14.6165/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval12.0568-14.6165/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_12.0568-14.6165.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval12.0568-14.6165/gll_ft1_tr_bn190114873_v00_filt.fit.........!
real 10.64
user 7.92
sys 2.65
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval12.0568-14.6165/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_12.0568-14.6165.xml
Optimizer: Minuit
Performing likelihood fit...
Data 9.0
srcName 2.576925063095601e-06
srcName 9.006156211128799
srcName 0.0031007134983776575
srcName 0.0007491254045130694
Resid 9.0 9.010008626956754 3.8994587198479653
plotting GRB spectrum
srcName 9.006156211128799
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 81|
| | Integral| 0.00272| 0.000952| ph./cm2/s| |
| | Index| -2.47| 0.445| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.2e-06| 5.16e-07| erg/cm2/s| |
| | Photon flux| 0.00272| 0.000952| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.101| 0.96| -| |
| | Energy flux| 1.2e-08| 1.14e-07| erg/cm2/s| |
| | Photon flux| 2.61e-05| 0.000247| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 30.555163567344433
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval12.0568-14.6165/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval12.0568-14.6165/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.32
user 6.37
sys 0.85
Interval # 19 (14.6165-17.7834):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_14.6165-17.7834.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='14.6165' tstop='17.7834' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192242.2425001 tstop=569192245.4094001 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192242.2425001 tmax=569192245.4094001 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_14.6165-17.7834.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 3.1669000387191772
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_14.6165-17.7834.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_14.6165-17.7834.xml 3.1669000387191772 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_14.6165-17.7834.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_14.6165-17.7834.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval14.6165-17.7834/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.96
user 0.37
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval14.6165-17.7834/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Starting calculation of region 20.0,0.0 to 40.0,40.0
Completed calculation of region 20.0,0.0 to 40.0,40.0
Starting calculation of region 0.0,0.0 to 20.0,40.0
Completed calculation of region 0.0,0.0 to 20.0,40.0
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
MIGRAD MINIMIZATION HAS CONVERGED.
FCN= 38.58473 FROM MIGRAD STATUS=CONVERGED 60 CALLS 61 TOTAL
EDM= .91E-05 STRATEGY=1 ERROR MATRIX UNCERTAINTY= 4.2%
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral 1.8976 .58104 .59088E-04 .20753
2 Index -1.7239 .28390 -.30977E-03 -.18372E-01
3 Value .99995 .14393 -.83818E-06 .21442E-05
4 Normalizat .10039 6.4295 -.61998 -.24045E-03
ERR DEF= .500
Final values:
Integral = 1.89763
Index = -1.7239
Value = 0.999953
Normalizat = 0.100385
**********
** 6 **HESSE
**********
FCN= 38.58473 FROM HESSE STATUS=OK 25 CALLS 86 TOTAL
EDM= .17E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral 1.8976 .58219 .80273E-05 -1.4836
2 Index -1.7239 .28427 .31391E-03 .43675
3 Value .99995 .14383 .30552E-03 -.15824E-03
4 Normalizat .10039 5.9882 .24419 -1.5833
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 1.65135e-05
Minuit parameter uncertainties:
1 0.582208
2 0.284786
3 0.15
4 0.446159
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 41.85635 FROM MIGRAD STATUS=CONVERGED 68 CALLS 69 TOTAL
EDM= .15E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral .72493 .22999 .12243E-02 .48816
2 Index -1.4209 .27207 .15251E-01 -.54589E-01
3 Value 1.0001 .14394 .72202E-01 .36621E-02
4 Normalizat .10260 9.8399 .45249 -.29768E-02
ERR DEF= .500
Final values:
Integral = 0.724934
Index = -1.42086
Value = 1.00009
Normalizat = 0.102597
**********
** 6 **HESSE
**********
FCN= 41.85635 FROM HESSE STATUS=OK 23 CALLS 92 TOTAL
EDM= .15E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral .72493 .22962 .54127E-05 -1.5169
2 Index -1.4209 .27166 .33726E-03 .55135
3 Value 1.0001 .14383 .15903E-02 .30814E-03
4 Normalizat .10260 9.8541 .10574E-01 -1.6032
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.000147899
Minuit parameter uncertainties:
1 0.229621
2 0.272168
3 0.15
4 0.528991
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval14.6165-17.7834/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_14.6165-17.7834.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval14.6165-17.7834/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 8.75
user 7.77
sys 0.93
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval14.6165-17.7834/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_14.6165-17.7834.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 10.005761086845931
srcName 0.0038360472130242905
srcName 0.0009197943074131136
Resid 10.0 10.010519505291432 -4.503365482686023
plotting GRB spectrum
srcName 10.005761086845931
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 122|
| | Integral| 0.00205| 0.000663| ph./cm2/s| |
| | Index| -1.78| 0.306| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 2.04e-06| 9.94e-07| erg/cm2/s| |
| | Photon flux| 0.002| 0.000663| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.1| 0.439| -| |
| | Energy flux| 1.19e-08| 5.2e-08| erg/cm2/s| |
| | Photon flux| 2.59e-05| 0.000113| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 29.319805156924488
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval14.6165-17.7834/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval14.6165-17.7834/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.18
user 6.37
sys 0.73
Interval # 20 (17.7834-21.4962):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_17.7834-21.4962.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='17.7834' tstop='21.4962' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192245.4094001 tstop=569192249.1222 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192245.4094001 tmax=569192249.1222 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 11 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_17.7834-21.4962.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.18
user 0.14
sys 0.03
Total number of events in the counts map: 11
Total time in Good Time Intervals: 3.712799906730652
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_17.7834-21.4962.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_17.7834-21.4962.xml 3.712799906730652 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_17.7834-21.4962.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_17.7834-21.4962.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval17.7834-21.4962/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.92
user 0.37
sys 0.44
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval17.7834-21.4962/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval17.7834-21.4962/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_17.7834-21.4962.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval17.7834-21.4962/gll_ft1_tr_bn190114873_v00_filt.fit...........!
real 8.51
user 7.51
sys 0.93
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval17.7834-21.4962/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_17.7834-21.4962.xml
Optimizer: Minuit
Performing likelihood fit...
Data 11.0
srcName 2.576925063095601e-06
srcName 11.006251480447592
srcName 0.004497229833929843
srcName 0.0010795093025735792
Resid 11.0 11.01183079650916 3.177759463810659
plotting GRB spectrum
srcName 11.006251480447592
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 133|
| | Integral| 0.0019| 0.000582| ph./cm2/s| |
| | Index| -1.72| 0.285| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 2.06e-06| 9.58e-07| erg/cm2/s| |
| | Photon flux| 0.00184| 0.000581| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.1| 0.446| -| |
| | Energy flux| 1.19e-08| 5.29e-08| erg/cm2/s| |
| | Photon flux| 2.59e-05| 0.000115| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 38.58473129896198
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval17.7834-21.4962/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval17.7834-21.4962/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.12
user 6.36
sys 0.70
Interval # 21 (21.4962-30.0798):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_21.4962-30.0798.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='21.4962' tstop='30.0798' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192249.1222 tstop=569192257.7058 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192249.1222 tmax=569192257.7058 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_21.4962-30.0798.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 10
Total time in Good Time Intervals: 8.583600044250488
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 40.63160 FROM MIGRAD STATUS=CONVERGED 71 CALLS 72 TOTAL
EDM= .94E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral .58377 .19045 .10825E-02 .72954
2 Index -1.2987 .26752 .14821E-01 -.36467E-01
3 Value .99973 .14394 .71150E-01 -.10590E-02
4 Normalizat .10135 9.8953 .44637 -.23524E-02
ERR DEF= .500
Final values:
Integral = 0.583774
Index = -1.2987
Value = 0.999725
Normalizat = 0.101347
**********
** 6 **HESSE
**********
FCN= 40.63160 FROM HESSE STATUS=OK 23 CALLS 95 TOTAL
EDM= .93E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral .58377 .18915 .47863E-05 -1.5225
2 Index -1.2987 .26575 .65595E-04 .59982
3 Value .99973 .14383 .15671E-02 -.91549E-03
4 Normalizat .10135 9.8981 .99439E-02 -1.5941
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 9.32998e-05
Minuit parameter uncertainties:
1 0.189149
2 0.266263
3 0.15
4 0.363662
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 34.58971 FROM MIGRAD STATUS=CONVERGED 73 CALLS 74 TOTAL
EDM= .11E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral .71691 .24355 .11682E-02 .20940
2 Index -1.3355 .28274 .14505E-01 -.17025E-01
3 Value .99986 .14392 .65717E-01 .47854E-03
4 Normalizat .10015 9.8414 .43531 -.69842E-03
ERR DEF= .500
Final values:
Integral = 0.716907
Index = -1.33552
Value = 0.999862
Normalizat = 0.100148
**********
** 6 **HESSE
**********
FCN= 34.58971 FROM HESSE STATUS=OK 23 CALLS 97 TOTAL
EDM= .12E-04 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral .71691 .24236 .51645E-05 -1.5172
2 Index -1.3355 .28142 .64190E-04 .58505
3 Value .99986 .14383 .14472E-02 -.45941E-03
4 Normalizat .10015 9.8547 .96945E-02 -1.5785
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 1.15059e-05
Minuit parameter uncertainties:
1 0.242366
2 0.282014
3 0.15
4 0.127125
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_21.4962-30.0798.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_21.4962-30.0798.xml 8.583600044250488 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_21.4962-30.0798.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_21.4962-30.0798.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval21.4962-30.0798/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
...!
real 0.98
user 0.37
sys 0.47
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval21.4962-30.0798/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Starting calculation of region 0.0,0.0 to 20.0,40.0
Completed calculation of region 0.0,0.0 to 20.0,40.0
Starting calculation of region 20.0,0.0 to 40.0,40.0
Completed calculation of region 20.0,0.0 to 40.0,40.0
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval21.4962-30.0798/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_21.4962-30.0798.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval21.4962-30.0798/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 8.05
user 7.25
sys 0.74
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval21.4962-30.0798/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_21.4962-30.0798.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 10.010640787432061
srcName 0.010187426096490185
srcName 0.0024970868626834467
Resid 10.0 10.0233278773163 -2.8054789536585467
plotting GRB spectrum
srcName 10.010640787432061
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 119|
| | Integral| 0.000725| 0.00023| ph./cm2/s| |
| | Index| -1.42| 0.272| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.2e-06| 5.71e-07| erg/cm2/s| |
| | Photon flux| 0.000656| 0.000215| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.103| 0.529| -| |
| | Energy flux| 1.22e-08| 6.27e-08| erg/cm2/s| |
| | Photon flux| 2.65e-05| 0.000136| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 41.856346424972635
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval21.4962-30.0798/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval21.4962-30.0798/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 6.57
user 5.79
sys 0.69
Interval # 22 (30.0798-40.8747):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_30.0798-40.8747.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='30.0798' tstop='40.8747' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192257.7058 tstop=569192268.5007 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192257.7058 tmax=569192268.5007 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.02
Selected 10 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_30.0798-40.8747.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.02
Total number of events in the counts map: 10
Total time in Good Time Intervals: 10.794899940490723
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_30.0798-40.8747.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_30.0798-40.8747.xml 10.794899940490723 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_30.0798-40.8747.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_30.0798-40.8747.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval30.0798-40.8747/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.91
user 0.36
sys 0.44
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval30.0798-40.8747/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval30.0798-40.8747/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_30.0798-40.8747.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval30.0798-40.8747/gll_ft1_tr_bn190114873_v00_filt.fit..........!
real 8.13
user 7.37
sys 0.73
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval30.0798-40.8747/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_30.0798-40.8747.xml
Optimizer: Minuit
Performing likelihood fit...
Data 10.0
srcName 2.576925063095601e-06
srcName 10.013614179002898
srcName 0.011990643824074353
srcName 0.0028972500543927764
Resid 10.0 10.028504649806429 -1.7529058518691403
plotting GRB spectrum
srcName 10.013614179002898
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 131|
| | Integral| 0.000584| 0.000189| ph./cm2/s| |
| | Index| -1.3| 0.266| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.11e-06| 5.17e-07| erg/cm2/s| |
| | Photon flux| 0.0005| 0.000163| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.000519| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.101| 0.364| -| |
| | Energy flux| 1.2e-08| 4.31e-08| erg/cm2/s| |
| | Photon flux| 2.61e-05| 9.38e-05| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 40.63160311031994
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 51.56070 FROM MIGRAD STATUS=CONVERGED 59 CALLS 60 TOTAL
EDM= .14E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral .33786 .10538 .88439E-03 -1.4505
2 Index -1.8426 .29898 .16674E-01 -.68750E-01
3 Value .99881 .14397 .80048E-01 -.10565E-01
4 Normalizat .10029 9.1445 .36933 -.20023E-02
ERR DEF= .500
Final values:
Integral = 0.337856
Index = -1.8426
Value = 0.998812
Normalizat = 0.100286
**********
** 6 **HESSE
**********
FCN= 51.56070 FROM HESSE STATUS=OK 23 CALLS 83 TOTAL
EDM= .14E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral .33786 .10544 .39116E-05 -1.5340
2 Index -1.8426 .29908 .36817E-03 .39358
3 Value .99881 .14383 .17635E-02 -.39603E-02
4 Normalizat .10029 9.1231 .82009E-02 -1.5815
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.000142591
Minuit parameter uncertainties:
1 0.105444
2 0.299662
3 0.150001
4 0.123166
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval30.0798-40.8747/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval30.0798-40.8747/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.09
user 6.34
sys 0.68
Interval # 23 (40.8747-48.7118):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_40.8747-48.7118.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='40.8747' tstop='48.7118' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192268.5007 tstop=569192276.3378 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192268.5007 tmax=569192276.3378 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 9 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_40.8747-48.7118.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 9
Total time in Good Time Intervals: 7.837100028991699
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_40.8747-48.7118.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_40.8747-48.7118.xml 7.837100028991699 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_40.8747-48.7118.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_40.8747-48.7118.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval40.8747-48.7118/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
..!
real 0.90
user 0.36
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval40.8747-48.7118/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval40.8747-48.7118/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_40.8747-48.7118.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval40.8747-48.7118/gll_ft1_tr_bn190114873_v00_filt.fit.........!
real 8.26
user 7.37
sys 0.82
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval40.8747-48.7118/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_40.8747-48.7118.xml
Optimizer: Minuit
Performing likelihood fit...
Data 9.0
srcName 2.576925063095601e-06
srcName 9.004502664663892
srcName 0.008706401606948282
srcName 0.0020785126302062273
Resid 9.0 9.015290155826113 -2.50769104874371
plotting GRB spectrum
srcName 9.004502664663892
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 126|
| | Integral| 0.000717| 0.000242| ph./cm2/s| |
| | Index| -1.34| 0.282| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 1.31e-06| 6.48e-07| erg/cm2/s| |
| | Photon flux| 0.000626| 0.000215| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 1| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.00052| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.1| 0.127| -| |
| | Energy flux| 1.19e-08| 1.51e-08| erg/cm2/s| |
| | Photon flux| 2.58e-05| 3.28e-05| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 34.589713913408474
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval40.8747-48.7118/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval40.8747-48.7118/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.07
user 6.23
sys 0.71
Interval # 24 (48.7118-73.7262):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_48.7118-73.7262.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='48.7118' tstop='73.7262' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192276.3378 tstop=569192301.3522 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.09
user 0.05
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192276.3378 tmax=569192301.3522 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.08
sys 0.03
Selected 11 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_48.7118-73.7262.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.03
Total number of events in the counts map: 11
Total time in Good Time Intervals: 25.014400005340576
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_48.7118-73.7262.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_48.7118-73.7262.xml 25.014400005340576 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_48.7118-73.7262.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_48.7118-73.7262.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval48.7118-73.7262/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
...!
real 0.92
user 0.38
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval48.7118-73.7262/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval48.7118-73.7262/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_48.7118-73.7262.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
**********
** 1 **SET PRINT .000
**********
**********
** 2 **SET NOWARN
**********
PARAMETER DEFINITIONS:
NO. NAME VALUE STEP SIZE LIMITS
1 'Integral ' .10000E-01 1.0000 .10000E-04 1000.0
2 'Index ' -2.0000 1.0000 -6.0000 .10000E-01
3 'Value ' 1.0000 1.0000 .70000 1.3000
4 'Normalizat' 1.0000 1.0000 .10000 10.000
**********
** 3 **SET ERR .5000
**********
**********
** 4 **SET GRAD 1.000
**********
**********
** 5 **MINIMIZE 900.0 2.000
**********
MIGRAD MINIMIZATION HAS CONVERGED.
MIGRAD WILL VERIFY CONVERGENCE AND ERROR MATRIX.
FCN= 66.71287 FROM MIGRAD STATUS=CONVERGED 64 CALLS 65 TOTAL
EDM= .42E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER STEP FIRST
NO. NAME VALUE ERROR SIZE DERIVATIVE
1 Integral .75329E-01 .33028E-01 .62594E-03 -3.0962
2 Index -1.8044 .37647 .23282E-01 -.46555E-01
3 Value .99940 .14401 .90951E-01 -.83283E-02
4 Normalizat 8.8533 8.7604 .45249 -.60690E-02
ERR DEF= .500
Final values:
Integral = 0.0753293
Index = -1.80438
Value = 0.999399
Normalizat = 8.85334
**********
** 6 **HESSE
**********
FCN= 66.71287 FROM HESSE STATUS=OK 23 CALLS 88 TOTAL
EDM= .42E-03 STRATEGY= 1 ERROR MATRIX ACCURATE
EXT PARAMETER INTERNAL INTERNAL
NO. NAME VALUE ERROR STEP SIZE VALUE
1 Integral .75329E-01 .35160E-01 .27722E-05 -1.5534
2 Index -1.8044 .38118 .51401E-03 .40739
3 Value .99940 .14383 .20043E-02 -.20047E-02
4 Normalizat 8.8533 8.2457 .24080E-02 .87626
ERR DEF= .500
Minuit fit quality: 3 estimated distance: 0.000417782
Minuit parameter uncertainties:
1 0.03516
2 0.382403
3 0.15
4 10.8336
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval48.7118-73.7262/gll_ft1_tr_bn190114873_v00_filt.fit...........!
real 10.12
user 9.29
sys 0.73
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval48.7118-73.7262/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_48.7118-73.7262.xml
Optimizer: Minuit
Performing likelihood fit...
Data 11.0
srcName 2.576925063095601e-06
srcName 10.963020541074815
srcName 0.02586463322104853
srcName 0.006173391514547778
Resid 11.0 10.995061142735473 -1.3024610428817343
plotting GRB spectrum
srcName 10.963020541074815
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 109|
| | Integral| 0.000338| 0.000105| ph./cm2/s| |
| | Index| -1.84| 0.3| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 3.09e-07| 1.42e-07| erg/cm2/s| |
| | Photon flux| 0.000332| 0.000106| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 0.999| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.000519| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 0|
| | Normalization| 0.1| 0.123| -| |
| | Energy flux| 1.19e-08| 1.46e-08| erg/cm2/s| |
| | Photon flux| 2.59e-05| 3.18e-05| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 51.56070495634684
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval48.7118-73.7262/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval48.7118-73.7262/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 7.04
user 6.22
sys 0.74
Interval # 25 (73.7262-172.5754):
-----------------------
-> gtdocountsmap.py rad='10.0' eventfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit' zmax='110.0' thetamax='180.0' emin='100.0' emax='100000.0' skymap='190114873_LAT_skymap_73.7262-172.5754.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' strategy='time' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' tstart='73.7262' tstop='172.5754' ra='54.51' dec='-26.939' irf='p8_transient020e' allowEmpty='no'
time -p gtmktime scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" filter="(DATA_QUAL>0 || DATA_QUAL==-1) && LAT_CONFIG==1 && IN_SAA!=T && LIVETIME>0 && (ANGSEP(RA_ZENITH,DEC_ZENITH,54.51,-26.939)<=(110.0-10.0))" roicut=no evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft1_tr_bn190114873_v00.fit evtable="EVENTS" outfile="gll_ft1_tr_bn190114873_v00_mkt.fit" apply_filter=yes overwrite=no header_obstimes=yes tstart=569192301.3522 tstop=569192400.2014 gtifile="default" chatter=2 clobber=yes debug=no gui=no mode="ql"
real 0.10
user 0.06
sys 0.03
Using 305 data
time -p gtselect infile=gll_ft1_tr_bn190114873_v00_mkt.fit outfile=gll_ft1_tr_bn190114873_v00_filt.fit ra=54.51 dec=-26.939 rad=10.0 tmin=569192301.3522 tmax=569192400.2014 emin=100.0 emax=100000.0 zmin=0.0 zmax=110.0 evclass=8 evtype=3 convtype=-1 phasemin=0.0 phasemax=1.0 evtable="EVENTS" chatter=2 clobber=yes debug=no gui=no mode="ql"
Done.
real 0.12
user 0.09
sys 0.03
Selected 9 events.
time -p gtbin evfile=gll_ft1_tr_bn190114873_v00_filt.fit scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit outfile=190114873_LAT_skymap_73.7262-172.5754.fit algorithm="CMAP" ebinalg="LOG" emin=30.0 emax=200000.0 ebinfile=NONE tbinalg="LIN" tbinfile=NONE nxpix=101 nypix=101 binsz=0.2 coordsys="CEL" xref=54.51 yref=-26.939 axisrot=0.0 rafield="RA" decfield="DEC" proj="AIT" hpx_ordering_scheme="RING" hpx_order=3 hpx_ebin=yes hpx_region="" evtable="EVENTS" sctable="SC_DATA" efield="ENERGY" tfield="TIME" chatter=2 clobber=yes debug=no gui=no mode="ql"
This is gtbin version HEAD
real 0.17
user 0.13
sys 0.02
Total number of events in the counts map: 9
Total time in Good Time Intervals: 98.84920001029968
-> gtbuildxmlmodel xmlmodel='190114873_LAT_xmlmodel_73.7262-172.5754.xml' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' galactic_model='template' particle_model='isotr template' ra='54.51' dec='-26.939' fgl_mode='fast' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' source_model='PowerLaw2'
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
addFGLsources( 54.51 -26.939 18.0 190114873_LAT_xmlmodel_73.7262-172.5754.xml 98.84920001029968 )
('SpatialMap', True)
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using template /usr/local/miniconda/envs/test_env/share/fermitools/data/pyBurstAnalysisGUI/templates/FornaxA.fits...
Keeping diffuse source 4FGL J0322.6-3712e (10.77 deg away) using spatial model SpatialMap...
Kept 1 point sources from the FGL catalog
-> gtdolike.py spectralfiles='no' xmlmodel='190114873_LAT_xmlmodel_73.7262-172.5754.xml' liketype='unbinned' filteredeventfile='gll_ft1_tr_bn190114873_v00_filt.fit' rspfile='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_cspec_tr_bn190114873_v00.rsp' showmodelimage='no' tsmin='20.0' optimizeposition='no' ft2file='/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit' skymap='190114873_LAT_skymap_73.7262-172.5754.fit' flemin='100.000000' flemax='10000.000000'
time -p gtltcube evfile="/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval73.7262-172.5754/gll_ft1_tr_bn190114873_v00_filt.fit" evtable="EVENTS" scfile=__ft2temp.fits sctable="SC_DATA" outfile=gll_ft1_tr_bn190114873_v00_filt_ltcube.fit dcostheta=0.025 binsz=1.0 phibins=1 tmin=0.0 tmax=0.0 file_version="1" zmin=0.0 zmax=180.0 chatter=2 clobber=yes debug=no gui=no mode="ql"
Working on file __ft2temp.fits
.....!
real 0.92
user 0.38
sys 0.45
/usr/local/miniconda/envs/test_env/lib/python3.9/site-packages/fermitools/GtBurst/gtapps_mp/gtexpmap_mp.py 40 40 2 1 /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval73.7262-172.5754/gll_ft1_tr_bn190114873_v00_filt.fit gll_ft1_tr_bn190114873_v00_filt_ltcube.fit P8R3_TRANSIENT020E_V3 20.0 20 gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Spawning 2 jobs...
Combining temporary files...
Deleting temporary files...
time -p gtdiffrsp evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval73.7262-172.5754/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" srcmdl=190114873_LAT_xmlmodel_73.7262-172.5754.xml irfs="P8R3_TRANSIENT020E_V3" evclsmin="INDEF" evclass="INDEF" evtype="INDEF" convert=no chatter=2 clobber=yes debug=no gui=no mode="ql"
adding source 4FGL J0322.6-3712e
adding source GalacticTemplate
adding source IsotropicTemplate
Working on...
/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval73.7262-172.5754/gll_ft1_tr_bn190114873_v00_filt.fit.........!
real 8.02
user 7.24
sys 0.70
Loading python Likelihood interface...
Applying a Gaussian prior with sigma 0.15 on the normalization of the Galactic Template
{'Norm': 1.0, 'Mean': 1.0, 'Sigma': 0.15, 'Offset': 0.0}
Likelihood settings:
Event file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval73.7262-172.5754/gll_ft1_tr_bn190114873_v00_filt.fit
Spacecraft file(s): /Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit
Exposure map: gll_ft1_tr_bn190114873_v00_filt_expomap.fit
Exposure cube: gll_ft1_tr_bn190114873_v00_filt_ltcube.fit
IRFs: P8R3_TRANSIENT020E_V3
Source model file: 190114873_LAT_xmlmodel_73.7262-172.5754.xml
Optimizer: Minuit
Performing likelihood fit...
Data 9.0
srcName 2.576925063095601e-06
srcName 7.198715859931537
srcName 0.08005093825016875
srcName 1.6745755553434722
Resid 9.0 8.95334493045024 -3.323470981883559
plotting GRB spectrum
srcName 7.198715859931537
|--------------------|---------------|----------| ----------|----------|------|
| Source name| Par. Name| Value| Error| Units| TS|
|--------------------|---------------|----------|------------|----------|------|
|GRB | | | | | 41|
| | Integral| 7.53e-05| 3.52e-05| ph./cm2/s| |
| | Index| -1.8| 0.382| -| |
| | LowerLimit| 100|n.a. (fixed)| MeV| |
| | UpperLimit| 1e+05|n.a. (fixed)| MeV| |
| | Energy flux| 7.28e-08| 4.15e-08| erg/cm2/s| |
| | Photon flux| 7.38e-05| 3.54e-05| ph./cm2/s| |
|GalacticTemplate | | | | | 0|
| | Value| 0.999| 0.15| -| |
| | Energy flux| 3.76e-07| 5.64e-08| erg/cm2/s| |
| | Photon flux| 0.000519| 7.79e-05| ph./cm2/s| |
|IsotropicTemplate | | | | | 1|
| | Normalization| 8.85| 10.8| -| |
| | Energy flux| 1.05e-06| 1.28e-06| erg/cm2/s| |
| | Photon flux| 0.00228| 0.00279| ph./cm2/s| |
--------------------------------------------------------------------------------
*** plus 1 FGL sources with TS<1 (not printed to save space)
*** All fluxes and upper limits have been computed in the 100.0 - 10000.0 energy range.
*** Upper limits (if any) are computed assuming a photon index of -2.0, with the 95.0 % c.l.
Log(likelihood) = 66.71287429892232
time -p gtsrcprob evfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval73.7262-172.5754/gll_ft1_tr_bn190114873_v00_filt.fit evtable="EVENTS" scfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/bn190114873/gll_ft2_tr_bn190114873_v00.fit sctable="SC_DATA" outfile=/Users/runner/work/threeML/threeML/docs/md_docs/slow_execute/interval73.7262-172.5754/gll_ft1_tr_bn190114873_v00_filt_prob.fit srcmdl=gll_ft1_tr_bn190114873_v00_filt_likeRes.xml irfs="CALDB" evtype="INDEF" srclist= chatter=2 clobber=yes debug=no gui=no mode="ql"
real 6.49
user 5.81
sys 0.65
00:38:36 INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval10.568-12.0568/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval12.0568-14.6165/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval14.6165-17.7834/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval17.7834-21.4962/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval2.6996-3.6358/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval21.4962-30.0798/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval3.6358-3.9968/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval3.9968-4.4024/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval30.0798-40.8747/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval4.4024-4.7375/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval4.7375-5.0909/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval40.8747-48.7118/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval48.7118-73.7262/gll_ft2_tr_bn190114873_v00.fit
00:38:37 INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval5.0909-5.5471/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval5.5471-5.9896/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval5.9896-6.3998/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval6.3998-6.6889/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval6.6889-7.0117/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval7.0117-7.2936/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval7.2936-7.7731/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval7.7731-8.2167/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval73.7262-172.5754/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval8.2167-8.8763/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval8.8763-9.6573/gll_ft2_tr_bn190114873_v00.fit
INFO The ft2 file does not exist. Please examine! lat_transient_builder.py:722
INFO we will grab the data file for you. lat_transient_builder.py:723
INFO copied ./bn190114873/gll_ft2_tr_bn190114873_v00.fit to lat_transient_builder.py:739 interval9.6573-10.568/gll_ft2_tr_bn190114873_v00.fit
At this point we can create the FermiLATLike plugins from each of the observation:
[13]:
LAT_plugins = {}
for l in LAT_observations:
LAT_name = "LAT_%06.3f-%06.3f" % (float(l.tstart), float(l.tstop))
LAT_plugins[LAT_name] = l.to_LATLike()
pass
For reference, these are the keys save in the dictionary.
[14]:
LAT_plugins.keys()
[14]:
dict_keys(['LAT_10.568-12.057', 'LAT_12.057-14.617', 'LAT_14.617-17.783', 'LAT_17.783-21.496', 'LAT_02.700-03.636', 'LAT_21.496-30.080', 'LAT_03.636-03.997', 'LAT_03.997-04.402', 'LAT_30.080-40.875', 'LAT_04.402-04.737', 'LAT_04.737-05.091', 'LAT_40.875-48.712', 'LAT_48.712-73.726', 'LAT_05.091-05.547', 'LAT_05.547-05.990', 'LAT_05.990-06.400', 'LAT_06.400-06.689', 'LAT_06.689-07.012', 'LAT_07.012-07.294', 'LAT_07.294-07.773', 'LAT_07.773-08.217', 'LAT_73.726-172.575', 'LAT_08.217-08.876', 'LAT_08.876-09.657', 'LAT_09.657-10.568'])
Now we can perform the fit in each bin. Note that we set the model, and we set some initial values. All the resulting joint likelihood objects are stored in a dictioonary to be used later for plotting.
[15]:
results = {}
update_logging_level("DEBUG")
for T0, T1 in zip(intervals[:-1], intervals[1:]):
GRB = PointSource(
"GRB", ra=myGRB["RA"], dec=myGRB["DEC"], spectral_shape=Powerlaw_flux()
)
model = Model(GRB)
model.GRB.spectrum.main.Powerlaw_flux.a = 100.0 * u.MeV
model.GRB.spectrum.main.Powerlaw_flux.b = 10000.0 * u.MeV
model.GRB.spectrum.main.Powerlaw_flux.F = 1.0
LAT_name = "LAT_%06.3f-%06.3f" % (T0, T1)
LAT_model_name = ("LAT%dX%d" % (T0, T1)).replace("-", "n")
datalist = DataList(LAT_plugins[LAT_name])
model["GRB.spectrum.main.Powerlaw_flux.F"].bounds = (1e-6, 1e6)
model["GRB.spectrum.main.Powerlaw_flux.F"].value = 1e-2
model["GRB.spectrum.main.Powerlaw_flux.index"].value = -2.2
model["GRB.spectrum.main.Powerlaw_flux.index"].bounds = (-3, 0)
jl = JointLikelihood(model, datalist, verbose=False)
model[LAT_model_name + "_GalacticTemplate_Value"].value = 1.0
model[LAT_model_name + "_GalacticTemplate_Value"].fix = True
model[LAT_model_name + "_GalacticTemplate_Value"].fix = True
# model.display( complete=True )
jl.set_minimizer("minuit")
jl.fit(compute_covariance=True)
results[LAT_name] = jl
pass
00:38:45 DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
00:38:45 DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:38:54 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:38:54 DEBUG adding child LAT2X3_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT2X3_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT2X3_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT2X3_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
00:38:55 DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -2.0352544023409047 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.99999999999764 minimization.py:802
DEBUG LAT2X3_IsotropicTemplate_Normalization = 1.4999999932566102 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 74.64 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
00:38:55 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT2X3_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT2X3_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT2X3_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT2X3_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (9.2 -2.5 +3.4) x 10^-3 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -3.0000000 +/- 0.0000018 | |
| LAT2X3_IsotropicTemplate_Normalization | 1.5000 +/- 0.0022 |
Correlation matrix:
| 1.00 | 0.00 | -0.00 |
| 0.00 | 1.00 | -0.00 |
| -0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT2X3 | 40.674435 |
| total | 40.674435 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 79.34887 |
| BIC | 81.34887 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:39:03 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:39:03 DEBUG adding child LAT3X3_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT3X3_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT3X3_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT3X3_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.6214002832513499 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.999999990196391 minimization.py:802
DEBUG LAT3X3_IsotropicTemplate_Normalization = 1.4999986085998898 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 75.24 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT3X3_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT3X3_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT3X3_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT3X3_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.4 -0.6 +0.9) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -3.00000 +/- 0.00010 | |
| LAT3X3_IsotropicTemplate_Normalization | 1.500 +/- 0.035 |
Correlation matrix:
| 1.00 | 0.00 | 0.00 |
| 0.00 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT3X3 | 29.524707 |
| total | 29.524707 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 57.049414 |
| BIC | 59.049414 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:39:11 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:39:11 DEBUG adding child LAT3X4_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT3X4_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT3X4_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT3X4_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.6740288325393682 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.9697989727745715 minimization.py:802
DEBUG LAT3X4_IsotropicTemplate_Normalization = 0.5000002063664295 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 73.68 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT3X4_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT3X4_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT3X4_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT3X4_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.1 -0.6 +0.8) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -3.0 +/- 0.5 | |
| LAT3X4_IsotropicTemplate_Normalization | (5.00 +/- 0.26) x 10^-1 |
Correlation matrix:
| 1.00 | -0.30 | 0.00 |
| -0.30 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT3X4 | 19.890601 |
| total | 19.890601 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 37.781202 |
| BIC | 39.781202 |
00:39:12 DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
00:39:12 DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:39:20 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:39:20 DEBUG adding child LAT4X4_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT4X4_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT4X4_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT4X4_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.6356358474267303 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.493350750381729 minimization.py:802
DEBUG LAT4X4_IsotropicTemplate_Normalization = 0.5000010514249715 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 55.94 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT4X4_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT4X4_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT4X4_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT4X4_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.3 -0.7 +0.9) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.5 +/- 0.4 | |
| LAT4X4_IsotropicTemplate_Normalization | (5.0 +/- 0.7) x 10^-1 |
Correlation matrix:
| 1.00 | -0.31 | 0.00 |
| -0.31 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT4X4 | 21.005797 |
| total | 21.005797 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 40.011593 |
| BIC | 42.011593 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:39:28 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:39:28 DEBUG adding child LAT4X5_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT4X5_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT4X5_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT4X5_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.6972341426974515 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.1561451176003112 minimization.py:802
DEBUG LAT4X5_IsotropicTemplate_Normalization = 0.5000012928966517 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 50.519999999999996 percent of samples have been thrown away because analysis_results.py:1739 they failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT4X5_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT4X5_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT4X5_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT4X5_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.0 -0.6 +0.8) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.2 +/- 0.4 | |
| LAT4X5_IsotropicTemplate_Normalization | (5.0 +/- 0.6) x 10^-1 |
Correlation matrix:
| 1.00 | -0.31 | 0.00 |
| -0.31 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT4X5 | 28.53492 |
| total | 28.53492 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 55.06984 |
| BIC | 57.06984 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:39:36 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:39:36 DEBUG adding child LAT5X5_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT5X5_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT5X5_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT5X5_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.9618894075014957 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.3571830585982771 minimization.py:802
DEBUG LAT5X5_IsotropicTemplate_Normalization = 0.5000000505896941 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
00:39:37 WARNING 51.080000000000005 percent of samples have been thrown away because analysis_results.py:1739 they failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
00:39:37 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT5X5_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT5X5_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT5X5_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT5X5_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.09 -0.32 +0.4) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.36 +/- 0.28 | |
| LAT5X5_IsotropicTemplate_Normalization | (5.00 +/- 0.14) x 10^-1 |
Correlation matrix:
| 1.00 | -0.25 | 0.00 |
| -0.25 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT5X5 | 24.17769 |
| total | 24.17769 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 46.355381 |
| BIC | 48.355381 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:39:45 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:39:45 DEBUG adding child LAT5X5_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT5X5_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT5X5_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT5X5_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.7988486401117976 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.124311369002779 minimization.py:802
DEBUG LAT5X5_IsotropicTemplate_Normalization = 0.5000216811989323 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 49.74 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT5X5_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT5X5_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT5X5_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT5X5_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.6 -0.4 +0.6) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.1 +/- 0.4 | |
| LAT5X5_IsotropicTemplate_Normalization | (5.0 +/- 2.2) x 10^-1 |
Correlation matrix:
| 1.00 | -0.31 | 0.00 |
| -0.31 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT5X5 | 22.737285 |
| total | 22.737285 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 43.474569 |
| BIC | 45.474569 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:39:53 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:39:53 DEBUG adding child LAT5X6_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT5X6_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT5X6_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT5X6_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.7205833403897994 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.517745472361178 minimization.py:802
DEBUG LAT5X6_IsotropicTemplate_Normalization = 1.1915964373561894 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
00:39:54 WARNING 53.300000000000004 percent of samples have been thrown away because analysis_results.py:1739 they failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
00:39:54 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT5X6_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT5X6_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT5X6_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT5X6_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.9 -0.5 +0.7) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.5 +/- 0.4 | |
| LAT5X6_IsotropicTemplate_Normalization | 1.2 +/- 0.7 |
Correlation matrix:
| 1.00 | -0.30 | -0.00 |
| -0.30 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT5X6 | 25.899097 |
| total | 25.899097 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 49.798193 |
| BIC | 51.798193 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:40:02 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:40:02 DEBUG adding child LAT6X6_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT6X6_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT6X6_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT6X6_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.5965227044098305 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.940019800051781 minimization.py:802
DEBUG LAT6X6_IsotropicTemplate_Normalization = 0.5000000003385661 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 50.1 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT6X6_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT6X6_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT6X6_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT6X6_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.5 -0.7 +0.9) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.94 +/- 0.31 | |
| LAT6X6_IsotropicTemplate_Normalization | (5.000 +/- 0.012) x 10^-1 |
Correlation matrix:
| 1.00 | -0.30 | 0.00 |
| -0.30 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT6X6 | 24.346972 |
| total | 24.346972 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 46.693944 |
| BIC | 48.693944 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:40:10 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:40:10 DEBUG adding child LAT6X7_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT6X7_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT6X7_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT6X7_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.6911011468022543 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.260509577977856 minimization.py:802
DEBUG LAT6X7_IsotropicTemplate_Normalization = 1.4999750447706044 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 55.44 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT6X7_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT6X7_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT6X7_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT6X7_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.0 -0.6 +0.9) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.3 +/- 0.4 | |
| LAT6X7_IsotropicTemplate_Normalization | 1.5 +/- 0.5 |
Correlation matrix:
| 1.00 | -0.31 | 0.00 |
| -0.31 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT6X7 | 21.119217 |
| total | 21.119217 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 40.238435 |
| BIC | 42.238435 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:40:18 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:40:18 DEBUG adding child LAT7X7_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT7X7_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT7X7_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT7X7_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
00:40:19 DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.6355787556887902 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.8762427213862418 minimization.py:802
DEBUG LAT7X7_IsotropicTemplate_Normalization = 0.5000026607773159 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 50.03999999999999 percent of samples have been thrown away because they analysis_results.py:1739 failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
00:40:19 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT7X7_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT7X7_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT7X7_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT7X7_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.3 -0.7 +0.9) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.88 +/- 0.32 | |
| LAT7X7_IsotropicTemplate_Normalization | (5.0 +/- 1.0) x 10^-1 |
Correlation matrix:
| 1.00 | -0.30 | -0.00 |
| -0.30 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT7X7 | 27.685109 |
| total | 27.685109 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 53.370219 |
| BIC | 55.370219 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:40:27 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:40:27 DEBUG adding child LAT7X7_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT7X7_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT7X7_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT7X7_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.8744278317060745 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.8169109932053746 minimization.py:802
DEBUG LAT7X7_IsotropicTemplate_Normalization = 0.5000000060552232 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 49.480000000000004 percent of samples have been thrown away because analysis_results.py:1739 they failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT7X7_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT7X7_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT7X7_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT7X7_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.3 -0.4 +0.5) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.82 +/- 0.31 | |
| LAT7X7_IsotropicTemplate_Normalization | (5.00 +/- 0.04) x 10^-1 |
Correlation matrix:
| 1.00 | -0.30 | 0.00 |
| -0.30 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT7X7 | 33.40629 |
| total | 33.40629 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 64.81258 |
| BIC | 66.81258 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:40:35 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:40:35 DEBUG adding child LAT7X8_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT7X8_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT7X8_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT7X8_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.7448000298623958 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.621535036513796 minimization.py:802
DEBUG LAT7X8_IsotropicTemplate_Normalization = 1.4997559272529473 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 60.3 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
00:40:36 DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT7X8_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT7X8_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT7X8_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT7X8_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.8 -0.5 +0.7) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.6 +/- 0.5 | |
| LAT7X8_IsotropicTemplate_Normalization | 1.5 +/- 0.5 |
Correlation matrix:
| 1.00 | -0.31 | -0.00 |
| -0.31 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT7X8 | 30.004254 |
| total | 30.004254 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 58.008508 |
| BIC | 60.008508 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
00:40:36 DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:40:44 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:40:44 DEBUG adding child LAT8X8_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT8X8_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT8X8_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT8X8_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.9668846079551272 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.1676492895104045 minimization.py:802
DEBUG LAT8X8_IsotropicTemplate_Normalization = 0.5000001067506735 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 51.519999999999996 percent of samples have been thrown away because analysis_results.py:1739 they failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT8X8_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT8X8_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT8X8_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT8X8_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.08 -0.31 +0.4) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.2 +/- 0.4 | |
| LAT8X8_IsotropicTemplate_Normalization | (5.00 +/- 0.17) x 10^-1 |
Correlation matrix:
| 1.00 | -0.31 | -0.00 |
| -0.31 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT8X8 | 28.291719 |
| total | 28.291719 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 54.583439 |
| BIC | 56.583439 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:40:52 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:40:52 DEBUG adding child LAT8X9_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT8X9_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT8X9_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT8X9_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -1.9981216797824937 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.1759721373894916 minimization.py:802
DEBUG LAT8X9_IsotropicTemplate_Normalization = 1.4999999990748192 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 50.68 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT8X9_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT8X9_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT8X9_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT8X9_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.00 -0.27 +0.4) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.18 +/- 0.35 | |
| LAT8X9_IsotropicTemplate_Normalization | 1.5000 +/- 0.0008 |
Correlation matrix:
| 1.00 | -0.31 | -0.00 |
| -0.31 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT8X9 | 42.093738 |
| total | 42.093738 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 82.187475 |
| BIC | 84.187475 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:41:00 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:41:00 DEBUG adding child LAT9X10_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT9X10_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT9X10_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT9X10_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -2.1665113563245555 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.728444394780525 minimization.py:802
DEBUG LAT9X10_IsotropicTemplate_Normalization = 1.499999995054957 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 49.14 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
00:41:01 DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT9X10_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT9X10_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT9X10_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT9X10_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (6.8 -1.9 +2.7) x 10^-3 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.73 +/- 0.30 | |
| LAT9X10_IsotropicTemplate_Normalization | 1.5000 +/- 0.0009 |
Correlation matrix:
| 1.00 | -0.29 | -0.00 |
| -0.29 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT9X10 | 43.35743 |
| total | 43.35743 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 84.714859 |
| BIC | 86.714859 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
00:41:01 DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:41:09 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:41:09 DEBUG adding child LAT10X12_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT10X12_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT10X12_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT10X12_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -2.415686253987546 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.46849894703508 minimization.py:802
DEBUG LAT10X12_IsotropicTemplate_Normalization = 1.4997336615722117 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 49.4 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT10X12_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT10X12_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT10X12_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT10X12_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (3.8 -1.1 +1.5) x 10^-3 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.47 +/- 0.28 | |
| LAT10X12_IsotropicTemplate_Normalization | 1.50 +/- 0.28 |
Correlation matrix:
| 1.00 | -0.27 | -0.00 |
| -0.27 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT10X12 | 44.700357 |
| total | 44.700357 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 87.400714 |
| BIC | 89.400714 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:41:17 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:41:17 DEBUG adding child LAT12X14_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT12X14_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT12X14_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT12X14_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -2.5668056304239846 minimization.py:802
00:41:18 DEBUG GRB.spectrum.main.Powerlaw_flux.index = -2.4717000458817178 minimization.py:802
DEBUG LAT12X14_IsotropicTemplate_Normalization = 0.500009523390559 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 56.04 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
00:41:18 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT12X14_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT12X14_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT12X14_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT12X14_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.7 -0.8 +1.1) x 10^-3 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.5 +/- 0.4 | |
| LAT12X14_IsotropicTemplate_Normalization | (5.0 +/- 0.9) x 10^-1 |
Correlation matrix:
| 1.00 | -0.31 | -0.00 |
| -0.31 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT12X14 | 43.357892 |
| total | 43.357892 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 84.715783 |
| BIC | 86.715783 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:41:26 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:41:26 DEBUG adding child LAT14X17_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT14X17_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT14X17_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT14X17_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -2.699540588239001 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.7821007118364733 minimization.py:802
DEBUG LAT14X17_IsotropicTemplate_Normalization = 1.473368589203411 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 46.52 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT14X17_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT14X17_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT14X17_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT14X17_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.0 -0.6 +0.8) x 10^-3 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.78 +/- 0.30 | |
| LAT14X17_IsotropicTemplate_Normalization | 1.47 +/- 0.23 |
Correlation matrix:
| 1.00 | -0.29 | -0.00 |
| -0.29 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT14X17 | 44.428195 |
| total | 44.428195 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 86.856389 |
| BIC | 88.856389 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
00:41:27 DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:41:34 DEBUG Removing non-needed files FermiLATLike.py:463
00:41:35 DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:41:35 DEBUG adding child LAT17X21_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT17X21_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT17X21_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT17X21_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -2.734846934332979 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.7232530642874537 minimization.py:802
DEBUG LAT17X21_IsotropicTemplate_Normalization = 0.5000013809483452 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 50.72 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT17X21_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT17X21_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT17X21_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT17X21_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (1.8 -0.5 +0.7) x 10^-3 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.72 +/- 0.28 | |
| LAT17X21_IsotropicTemplate_Normalization | (5.00 +/- 0.27) x 10^-1 |
Correlation matrix:
| 1.00 | -0.29 | 0.00 |
| -0.29 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT17X21 | 56.088597 |
| total | 56.088597 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 110.177194 |
| BIC | 112.177194 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:41:43 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:41:43 DEBUG adding child LAT21X30_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT21X30_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT21X30_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT21X30_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -3.18371726509655 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.4191892466200606 minimization.py:802
DEBUG LAT21X30_IsotropicTemplate_Normalization = 0.5000002428287336 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 49.919999999999995 percent of samples have been thrown away because analysis_results.py:1739 they failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT21X30_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT21X30_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT21X30_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT21X30_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (6.6 -1.8 +2.5) x 10^-4 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.42 +/- 0.27 | |
| LAT21X30_IsotropicTemplate_Normalization | (5.00 +/- 0.05) x 10^-1 |
Correlation matrix:
| 1.00 | -0.26 | -0.00 |
| -0.26 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT21X30 | 56.968107 |
| total | 56.968107 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 111.936213 |
| BIC | 113.936213 |
00:41:44 DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
00:41:44 DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:41:52 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:41:52 DEBUG adding child LAT30X40_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT30X40_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT30X40_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT30X40_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -3.302460651418001 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.2976855834223977 minimization.py:802
DEBUG LAT30X40_IsotropicTemplate_Normalization = 0.5000000007958773 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 49.559999999999995 percent of samples have been thrown away because analysis_results.py:1739 they failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT30X40_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT30X40_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT30X40_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT30X40_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (5.0 -1.4 +1.9) x 10^-4 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.30 +/- 0.27 | |
| LAT30X40_IsotropicTemplate_Normalization | (5.0000 +/- 0.0028) x 10^-1 |
Correlation matrix:
| 1.00 | -0.23 | -0.00 |
| -0.23 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT30X40 | 55.744111 |
| total | 55.744111 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 109.488222 |
| BIC | 111.488222 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:42:00 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:42:00 DEBUG adding child LAT40X48_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT40X48_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT40X48_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT40X48_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -3.204048274350687 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.3350359235393494 minimization.py:802
DEBUG LAT40X48_IsotropicTemplate_Normalization = 0.5000311056848792 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 50.63999999999999 percent of samples have been thrown away because they analysis_results.py:1739 failed the constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
00:42:01 DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT40X48_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT40X48_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT40X48_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT40X48_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (6.3 -1.8 +2.6) x 10^-4 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.34 +/- 0.28 | |
| LAT40X48_IsotropicTemplate_Normalization | (5.0 +/- 0.6) x 10^-1 |
Correlation matrix:
| 1.00 | -0.24 | -0.00 |
| -0.24 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT40X48 | 47.398842 |
| total | 47.398842 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 92.797685 |
| BIC | 94.797685 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
00:42:01 DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:42:09 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:42:09 DEBUG adding child LAT48X73_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT48X73_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT48X73_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT48X73_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -3.4787231739619373 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.8401675396308024 minimization.py:802
DEBUG LAT48X73_IsotropicTemplate_Normalization = 0.5000005651838437 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
WARNING 49.58 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT48X73_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT48X73_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT48X73_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT48X73_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (3.3 -0.9 +1.2) x 10^-4 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.84 +/- 0.30 | |
| LAT48X73_IsotropicTemplate_Normalization | (5.00 +/- 0.06) x 10^-1 |
Correlation matrix:
| 1.00 | -0.32 | -0.01 |
| -0.32 | 1.00 | 0.01 |
| -0.01 | 0.01 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT48X73 | 69.078036 |
| total | 69.078036 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 136.156071 |
| BIC | 138.156071 |
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
WARNING We have set the min_value of GRB.spectrum.main.Powerlaw_flux.F to 1e-99 because parameter.py:688 there was a postive transform
DEBUG creating new MLE analysis joint_likelihood.py:69
DEBUG REGISTERING MODEL joint_likelihood.py:119
Found Isotropic template for irf P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/iso_P8R3_TRANSIENT020E_V3_v1.txt
Found Galactic template for IRF. P8R3_TRANSIENT020E_V3: /usr/local/miniconda/envs/test_env/share/fermitools/refdata/fermi/galdiffuse/gll_iem_v07.fits
Cutting the template around the ROI:
00:42:17 DEBUG Removing non-needed files FermiLATLike.py:463
DEBUG removed {self._lmc._unique_filename} FermiLATLike.py:467
DEBUG removed {xml_file} FermiLATLike.py:471
DEBUG removed {temp_file} FermiLATLike.py:478
00:42:17 DEBUG adding child LAT73X172_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT73X172_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT73X172_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT73X172_IsotropicTemplate_Normalization node_type.py:180
DEBUG MODEL REGISTERED! joint_likelihood.py:144
INFO set the minimizer to minuit joint_likelihood.py:1043
INFO set the minimizer to MINUIT joint_likelihood.py:1060
DEBUG beginning the fit! joint_likelihood.py:234
DEBUG starting local optimization joint_likelihood.py:315
DEBUG Restoring best fit: minimization.py:796
DEBUG GRB.spectrum.main.Powerlaw_flux.F = -4.051371088724547 minimization.py:802
DEBUG GRB.spectrum.main.Powerlaw_flux.index = -1.8672738886792979 minimization.py:802
DEBUG LAT73X172_IsotropicTemplate_Normalization = 1.4998659199599225 minimization.py:802
WARNING get_number_of_data_points not implemented, values for statistical plugin_prototype.py:128 measurements such as AIC or BIC are unreliable
00:42:18 WARNING 49.02 percent of samples have been thrown away because they failed the analysis_results.py:1739 constraints on the parameters. This results might not be suitable for error propagation. Enlarge the boundaries until you loose less than 1 percent of the samples.
00:42:18 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT73X172_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT73X172_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT73X172_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT73X172_IsotropicTemplate_Normalization node_type.py:180
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (8.9 -2.8 +4) x 10^-5 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -1.87 +/- 0.35 | |
| LAT73X172_IsotropicTemplate_Normalization | 1.50 +/- 0.06 |
Correlation matrix:
| 1.00 | -0.36 | -0.00 |
| -0.36 | 1.00 | 0.00 |
| -0.00 | 0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT73X172 | 79.798931 |
| total | 79.798931 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 157.597862 |
| BIC | 159.597862 |
You can usethis function to graphically display the results of your fit (folded model, data and residuals)
[16]:
i = 3
T0, T1 = intervals[i], intervals[i + 1]
LAT_name = "LAT_%06.3f-%06.3f" % (T0, T1)
jl = results[LAT_name]
jl.results.display()
display_spectrum_model_counts(jl, step=False, figsize=(10, 10))
Best fit values:
| result | unit | |
|---|---|---|
| parameter | ||
| GRB.spectrum.main.Powerlaw_flux.F | (2.3 -0.7 +0.9) x 10^-2 | 1 / (cm2 s) |
| GRB.spectrum.main.Powerlaw_flux.index | -2.5 +/- 0.4 | |
| LAT4X4_IsotropicTemplate_Normalization | (5.0 +/- 0.7) x 10^-1 |
Correlation matrix:
| 1.00 | -0.31 | 0.00 |
| -0.31 | 1.00 | -0.00 |
| 0.00 | -0.00 | 1.00 |
Values of -log(likelihood) at the minimum:
| -log(likelihood) | |
|---|---|
| LAT4X4 | 21.005797 |
| total | 21.005797 |
Values of statistical measures:
| statistical measures | |
|---|---|
| AIC | 40.011593 |
| BIC | 42.011593 |
[16]:
We can see the evolution of the spectrum with time (not all the bins are diplayed):
[17]:
fig = plot_spectra(
*[results[k].results for k in list(results.keys())[::2]],
ene_min=100 * u.MeV,
ene_max=10 * u.GeV,
flux_unit="erg2/(cm2 s MeV)",
energy_unit="MeV",
fit_cmap="viridis",
contour_cmap="viridis",
contour_style_kwargs=dict(alpha=0.1)
)
fig.set_size_inches(10, 10)
00:42:20 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT2X3_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT2X3_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT2X3_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT2X3_IsotropicTemplate_Normalization node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT3X4_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT3X4_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT3X4_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT3X4_IsotropicTemplate_Normalization node_type.py:180
DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
DEBUG path is now: Powerlaw_flux.b node_type.py:180
DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
DEBUG adding child position node_type.py:89
DEBUG path is now: GRB.position node_type.py:180
DEBUG adding child main node_type.py:89
DEBUG path is now: spectrum.main node_type.py:180
DEBUG adding child spectrum node_type.py:89
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DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT7X8_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT7X8_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT7X8_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT7X8_IsotropicTemplate_Normalization node_type.py:180
00:44:29 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
DEBUG adding child a node_type.py:89
DEBUG path is now: Powerlaw_flux.a node_type.py:180
DEBUG adding child b node_type.py:89
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DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
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DEBUG path is now: main.polarization node_type.py:180
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DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
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DEBUG adding child LAT8X9_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT8X9_GalacticTemplate_Value node_type.py:180
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DEBUG path is now: LAT8X9_IsotropicTemplate_Normalization node_type.py:180
00:44:50 DEBUG adding child ra node_type.py:89
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DEBUG path is now: position.dec node_type.py:180
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DEBUG path is now: Powerlaw_flux.F node_type.py:180
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DEBUG path is now: Powerlaw_flux.index node_type.py:180
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DEBUG path is now: Powerlaw_flux.a node_type.py:180
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DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
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DEBUG path is now: GRB.position node_type.py:180
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DEBUG adding child spectrum node_type.py:89
DEBUG path is now: GRB.spectrum node_type.py:180
DEBUG adding child GRB node_type.py:89
DEBUG path is now: GRB node_type.py:180
DEBUG adding child LAT10X12_GalacticTemplate_Value node_type.py:89
DEBUG path is now: LAT10X12_GalacticTemplate_Value node_type.py:180
DEBUG adding child LAT10X12_IsotropicTemplate_Normalization node_type.py:89
DEBUG path is now: LAT10X12_IsotropicTemplate_Normalization node_type.py:180
00:45:11 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
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DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
DEBUG adding child polarization node_type.py:89
DEBUG path is now: main.polarization node_type.py:180
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DEBUG path is now: LAT14X17_IsotropicTemplate_Normalization node_type.py:180
00:45:33 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
DEBUG adding child dec node_type.py:89
DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
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DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
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DEBUG path is now: main.polarization node_type.py:180
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DEBUG adding child spectrum node_type.py:89
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DEBUG adding child LAT21X30_GalacticTemplate_Value node_type.py:89
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DEBUG path is now: LAT21X30_IsotropicTemplate_Normalization node_type.py:180
00:45:53 DEBUG adding child ra node_type.py:89
DEBUG path is now: position.ra node_type.py:180
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DEBUG path is now: position.dec node_type.py:180
DEBUG adding child F node_type.py:89
DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
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DEBUG path is now: LAT40X48_IsotropicTemplate_Normalization node_type.py:180
00:46:14 DEBUG adding child ra node_type.py:89
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DEBUG path is now: position.dec node_type.py:180
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DEBUG path is now: Powerlaw_flux.F node_type.py:180
DEBUG adding child index node_type.py:89
DEBUG path is now: Powerlaw_flux.index node_type.py:180
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DEBUG path is now: Powerlaw_flux.a node_type.py:180
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DEBUG adding child Powerlaw_flux node_type.py:89
DEBUG path is now: main.Powerlaw_flux node_type.py:180
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DEBUG path is now: main.polarization node_type.py:180
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00:46:35 DEBUG converting MeV to MeV model_plot.py:890
Finally, we can display flux lightcurves and index evolution with time.
[18]:
variates = ["F", "index"]
y = {}
for n in variates:
y[n] = []
y[n + "_p"] = []
y[n + "_n"] = []
x = []
dx = []
for T0, T1 in zip(intervals[:-1], intervals[1:]):
LAT_name = "LAT_%06.3f-%06.3f" % (T0, T1)
x.append((T1 + T0) / 2)
dx.append((T1 - T0) / 2)
jl = results[LAT_name]
res = jl.results
mod = res.optimized_model
ps = mod.point_sources
for n in variates:
my_variate = res.get_variates("GRB.spectrum.main.Powerlaw_flux.%s" % n)
y[n].append(my_variate.median)
y[n + "_p"].append(my_variate.equal_tail_interval()[1] - my_variate.median)
y[n + "_n"].append(my_variate.median - my_variate.equal_tail_interval()[0])
pass
pass
fig = plt.figure(figsize=(10, 15))
colors = ["r", "b"]
ylabels = ["Flux [100MeV - 10GeV] \n $\gamma$ cm$^{-2}$ s$^{-1}$", "index"]
for i, n in enumerate(variates):
plt.subplot(len(variates) + 1, 1, i + 1)
plt.errorbar(x, y[n], xerr=dx, yerr=(y[n + "_n"], y[n + "_p"]), ls="", c=colors[i])
if i == 0:
plt.yscale("log")
# plt.xscale('log')
plt.ylabel(ylabels[i])
pass
00:46:36 DEBUG adding child ra node_type.py:89
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DEBUG path is now: main.polarization node_type.py:180
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DEBUG path is now: Powerlaw_flux.F node_type.py:180
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DEBUG path is now: Powerlaw_flux.index node_type.py:180
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DEBUG path is now: Powerlaw_flux.F node_type.py:180
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00:46:37 DEBUG path is now: position.ra node_type.py:180
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DEBUG path is now: main.polarization node_type.py:180
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DEBUG path is now: LAT73X172_IsotropicTemplate_Normalization node_type.py:180
